The galaxy appears as an elliptical or lenticular system, exhibiting a relatively smooth, centrally concentrated light distribution. There is a discernible bulge component that dominates the overall morphology. The galaxy appears to have a moderate ellipticity, with its shape deviating somewhat from perfectly circular. The color profile suggests a population of older stars, contributing to its yellowish-red hue. There's no prominent evidence of spiral arms or significant dust lanes. The galaxy does not appear to be undergoing any major mergers or tidal interactions, although there is the possibility of a very slight irregularity.
