The galaxy presents a generally elliptical morphology, with the major axis oriented horizontally in the image. A distinct central bulge is apparent, exhibiting a concentrated, bright white luminosity. Circumscribing the bulge is a diffuse, somewhat indistinct disk. There are very faint spiral arm structures visible in the surrounding disk, contributing to its irregular appearance.

The color profile suggests varying stellar populations. The central bulge appears to be dominated by older stars, indicated by a redder hue, while the disk shows bluer tones, possibly due to the presence of younger stars. The galaxy lacks any immediately obvious tidal tails or signs of ongoing major merger activity, though subtle disturbances in the disk's symmetry could potentially indicate past minor interactions.
