The galaxy presents as a relatively compact, yet luminous object. Its overall shape is elliptical or spheroid, with a smooth, diffuse light distribution, suggesting a lack of prominent spiral arms or a well-defined disk. The core is characterized by a bright, concentrated central bulge. It exhibits a blue-ish hue surrounding the central region, possibly indicative of recent or ongoing star formation. Within this region, faint traces of dust lanes can be observed, although they are not distinctly separated from the main body of the galaxy. The galaxy appears to be relatively undisturbed, lacking any clear signs of major interactions or mergers. There is a subtle distortion in shape, indicative of potential minor disturbances.
