The galaxy presents a largely smooth and featureless morphology, indicative of an elliptical or lenticular type. Its light is centrally concentrated with a gradual decline in surface brightness moving outwards. The core appears bright and unresolved. There is a marginal flattening to the isophotes, exhibiting a generally elliptical shape. The color profile suggests an evolved stellar population, with a dominant yellowish-red hue. This is suggestive of older stars and a lack of significant ongoing star formation within the galaxy. There are no indications of spiral arms, dust lanes, or other distinct features usually associated with spiral galaxies. Faint extensions exist beyond the core, indicating a substantial halo component. There are no indications of tidal disturbances or recent merger activity. Overall, the galaxy appears as a quiescent, well-formed system.
