The galaxy presents an overall elliptical morphology, highly inclined relative to our line of sight, appearing as a flattened disk. There is a distinct central bulge region that appears bright and concentrated. The color profile suggests a generally redder population, indicative of older stars within the bulge. A relatively faint disk component surrounds the bulge, exhibiting a bluer hue, suggesting the presence of younger stars and potentially ongoing star formation. There is also a hint of asymmetry or minor disturbance in the overall structure, possibly due to a minor interaction or recent merger. The outer edges of the galaxy are somewhat diffuse, with evidence of faint tidal features or extended stellar halos.
