The galaxy presents as a centrally concentrated, smooth system. Its overall morphology is elliptical, exhibiting a high degree of central light concentration that gradually diminishes towards the outer regions. The light distribution appears to be relatively even across the galaxy's body. There is little evidence of spiral arms or significant dust lanes within the galaxy, lending to its classification as a relatively featureless system. Faint disturbances in the structure of the outer halo may be present. The galaxy displays a slightly elongated shape. The observed color suggests a population dominated by older stars, with a higher proportion of redder stars. This conclusion is based on the dominant orange-yellow hue exhibited by the galaxy, an indicator of aged stellar populations.
