The galaxy presents as a somewhat elliptical, though largely amorphous, structure. Its light is primarily concentrated in a central region, with a gradual decrease in luminosity towards the outer edges, suggesting an absence of well-defined spiral arms or a prominent disk. The central region appears to be dominated by older stars, emitting light in the redder bands, with hints of bluer regions indicative of ongoing or recent star formation. The galaxy appears moderately red in color, indicating a population of older stars and potentially a relatively low rate of current star formation. There are indications of minor disturbances within the galaxy's structure, potentially suggestive of a minor interaction or past merger event.
