The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a bright, concentrated luminosity profile, suggesting a well-defined nucleus or bulge. The light distribution fades gradually outwards from the core, with no apparent spiral arm structure or prominent dust lanes visible. The galaxy exhibits a yellow-reddish hue overall. The galaxy appears relatively isolated, with no obvious signs of ongoing major mergers or strong tidal interactions. However, there seems to be minor disturbances occurring. It is likely a high mass galaxy with relatively low star formation. 
