The galaxy presents as a roughly elliptical structure with a brighter, more condensed central region indicative of a galactic bulge. The galaxy exhibits a generally smooth texture, but some faint features or disturbances can be noted. It appears to be a spiral or lenticular galaxy seen from an angle that is not face-on. The overall color profile suggests a mix of stellar populations. The inner region appears bluer, possibly suggesting ongoing star formation, while the outer regions seem to be dominated by older, redder stars. No strong evidence of a major ongoing merger is immediately apparent, although some minor asymmetries or tidal features are observed.
