The galaxy presents as a moderately luminous, primarily smooth object. It exhibits an elliptical morphology, appearing to be in an intermediate state between perfectly round and elongated.  There are subtle indications of possible minor disturbances in its overall structure, but no signs of a major merger event are observed.  The galaxy's color profile indicates a population of older stars, with a relatively low rate of ongoing star formation. The color distribution within the galaxy appears fairly uniform, lacking any distinct blue regions that would typically indicate active star-forming regions. The galaxy exhibits a central concentration of light, which likely corresponds to the galactic bulge. Overall, it appears to be a relatively massive system.
