The galaxy presents as a relatively smooth, centrally concentrated object. The light profile appears to be dominated by a spheroidal component, showing a gradual decrease in luminosity from the core outwards.  There is a slight elongation, with the major axis oriented in a roughly horizontal direction. The galaxy appears to be largely featureless, lacking any prominent spiral arms or bar structures. The color index indicates a redder hue towards the core, which could suggest an older stellar population or dust obscuration in the central regions.  Fainter, bluer regions seem to be present in the outer parts, perhaps indicating some ongoing, albeit limited, star formation. There is no obvious evidence of any major ongoing mergers or strong tidal disturbances, though there are subtle asymmetries which may indicate minor past interactions.
