The galaxy appears as a centrally concentrated object with a smooth, diffuse morphology. There is a bright, somewhat amorphous central bulge that dominates the visual appearance. Surrounding the bulge is a fainter, more extended halo or disk component. The color profile suggests an older stellar population with a predominantly red-yellow hue in the central regions, transitioning to a slightly bluer tinge in the outer regions. The overall shape is generally round with a relatively smooth texture which shows no evidence of spiral arms or significant dust lanes. There are no obvious signs of major disturbances, such as tidal tails or strong asymmetries, that would indicate recent merger activity, although there is a slight clumping towards one side. The light distribution indicates it is likely an elliptical galaxy, or a lenticular galaxy viewed close to face-on.
