The galaxy presents as a moderately sized, face-on spiral with a distinct structure. Spiral arms are visible, exhibiting a somewhat patchy morphology which may indicate active star formation regions. The galaxy's bulge is noticeable, appearing as a concentrated central region with a yellowish hue, possibly suggestive of an older stellar population. A faint bar structure can be inferred running through the bulge. The galaxy's disk component is clearly observed, with the spiral arms extending outwards from the central region. No signs of tidal disturbances or major mergers are immediately apparent, suggesting that the galaxy is relatively undisturbed. The overall color suggests a mix of stellar populations.
