The galaxy presents a predominantly smooth morphology, with a slight asymmetry in its structure. The central region exhibits a concentrated luminosity, suggesting a significant stellar population or active galactic nucleus. The color appears to be skewed towards the redder end of the spectrum, consistent with an older stellar population. A faint, bluish extension is apparent on one side, possibly indicative of a minor tidal interaction or ongoing star formation. The overall shape is somewhere between round and elliptical, although it's difficult to fully determine with the image quality.
