The galaxy presents as a relatively small, disk-shaped structure, seemingly viewed at a high inclination. A prominent dust lane appears to bisect the galaxy's central region, obscuring some of the light. The overall color profile suggests a mix of stellar populations. Blue hues are present in the outer edges and a concentrated area toward one side of the galaxy, possibly indicating recent star formation within spiral arms. Some areas toward the other side of the galaxy have a redder color, perhaps indicating the presence of an older stellar population or significant dust extinction. There is a brighter area near the end that may be a region of active star formation. The luminosity appears to be concentrated toward the central bulge, though not overwhelmingly so. There may be very faint hints of a distorted structure or tidal features, which could suggest past or ongoing interactions with another galaxy, but these are subtle and require further investigation. The outer regions appear fainter and less defined, making it difficult to discern the precise extent of the galactic disk.
