The galaxy presents as a somewhat diffuse and moderately luminous object. Its general morphology appears elliptical, exhibiting a relatively smooth profile without prominent spiral arms or a well-defined disk structure. The central region displays a high concentration of light, suggesting a substantial bulge component. This core is yellowish in color, potentially indicative of an older stellar population and reduced ongoing star formation activity. The outer regions fade gradually into the background, with hints of bluer light, possibly signifying younger stars or some residual star formation in these areas. There is some evidence of tidal disturbances and potentially minor merging events.
