The galaxy presents as an elliptical morphology, exhibiting a relatively smooth light distribution with no readily apparent spiral arm structures. The overall color appears yellowish-white, suggesting a stellar population dominated by older, lower-mass stars. The galaxy displays a central concentration of light, possibly indicating a bulge component, or an active galactic nucleus. There is no obvious presence of ongoing major star formation within the galaxy. The shape is generally round, with only minor deviations from circular symmetry. There are no apparent signs of significant tidal disturbances or ongoing merging activity, though minor disturbances cannot be fully ruled out.
