The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge that is bright and slightly yellow, indicating an older stellar population within the core. The surrounding disk appears elongated, with a color gradient transitioning from yellow to bluish hues further from the center. This implies a possible presence of younger, hotter stars and ongoing star formation in the outer regions, contrasting with the older population in the core. There is little evidence of defined spiral arms. Slight asymmetry or minor disturbances may be present in the outer regions. Overall, the galaxy appears relatively isolated and not strongly interacting with any other objects in its immediate vicinity.
