The galaxy presents as a relatively smooth, featureless elliptical or lenticular-type system. It exhibits an overall elongated, cigar-like shape. A prominent central bulge dominates the visual structure, displaying a concentrated, yellowish hue, suggesting an older stellar population. The disk, if present, is not well-defined, with the light gradually fading from the central bulge towards the outer edges of the galaxy. There are no immediately apparent signs of significant ongoing star formation or recent mergers. The overall color profile indicates a predominantly evolved stellar population with limited blue emission associated with younger stars. The lack of distinct spiral arms or irregular structures suggests a quiescent system.
