The galaxy appears to be a relatively compact and luminous object. It exhibits a smooth, somewhat elliptical morphology, with no readily apparent spiral arms or distinct features such as bars or rings. The galaxy's light is concentrated towards the center, suggesting a substantial bulge component. The color profile seems fairly uniform across the galaxy, trending towards the redder end of the spectrum. This redder color suggests a stellar population dominated by older, less massive stars, with comparatively little ongoing star formation. There is no indication of strong tidal features or morphological disturbances, suggesting it is not undergoing a major merger or strong gravitational interaction currently. The object does show a slight elongation, deviating from a perfectly circular shape.
