The galaxy presents as a luminous, somewhat amorphous structure, appearing predominantly smooth in texture. It exhibits a generally rounded morphology, although some elongation is present. The color profile suggests a population of older stars, biased towards the redder end of the spectrum, with a lack of distinct blue star-forming regions. The galaxy displays evidence of potential interaction or a recent merger event. A clear structure is difficult to define; overall the light distribution has an asymmetrical profile, perhaps with some substructure.
