This galaxy presents as a relatively smooth, elongated structure with a bright central bulge. The overall color appears to be trending towards the redder end of the spectrum, though there are subtle variations across the galaxy's body with bluer colors appearing on the outer edges. The morphology suggests a possible early-type spiral galaxy, potentially an Sa or Sb, where star formation activity is not as prominent as later-type spirals. The light is concentrated towards the center, indicating a dominant, older stellar population with a significant amount of internal dust obscuring some of the light. No obvious spiral arm structures are visible, possibly due to the inclination or the smoothing effect of distance and resolution, but the overall structure seems fairly undisturbed, without any major signs of tidal interactions or recent merger activity.
