The galaxy presents as a relatively smooth, elongated structure, likely an elliptical galaxy or a lenticular galaxy seen at an oblique angle. A bright central bulge dominates the galaxy's luminosity profile, exhibiting a yellowish-white hue, suggesting an older stellar population. The outer regions fade gradually, with a less defined edge. There is little evidence of spiral arm structure or significant dust lanes, indicating a lack of ongoing or recent major star formation. There may be some very faint features indicating tidal interactions or minor disturbances. The color gradient suggests a transition from older, redder stars in the central bulge to potentially slightly younger, bluer stars in the outer disk or halo, although this difference is subtle. Overall, the galaxy appears to be a passively evolving system of considerable mass, with a high degree of central concentration.
