The galaxy presents as a somewhat elongated, lenticular object. The central bulge region appears relatively smooth and concentrated, exhibiting a moderate degree of symmetry, though slightly askew. A subtle disk component can be inferred, presenting as a faint, nebulous extension. The overall color profile suggests an older stellar population, and there is no evident spiral arm structure or significant dust lane obscuration. There appears to be a slight color gradient that may indicate the presence of star formation within. There is some possibility of a minor disturbance.
