The galaxy presents a primarily smooth, elliptical morphology, appearing somewhat elongated in shape. A bright central bulge dominates the structure, with the luminosity decreasing gradually towards the outer edges of the galaxy. The color profile indicates a relatively older stellar population, exhibiting a yellowish-red hue indicative of evolved stars. There is minimal evidence of spiral arm structure or significant dust lanes within the visible spectrum. Subtle irregularities or minor disturbances are potentially present in the outer regions, but these are not pronounced enough to indicate a recent major merger. Overall, the galaxy appears to be a relatively evolved system, likely in the process of quiescence.
