The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology is elliptical, exhibiting a notable lack of spiral arm structure. The light profile gradually fades from a bright, yellowish core towards the outer edges, suggesting a population of older stars dominating the light emission. There's a subtle color gradient within the galaxy; the core appears slightly more yellow, possibly indicating a higher concentration of older, redder stars or dust. The outer regions seem slightly bluer, potentially hinting at a small amount of ongoing star formation. No significant tidal features or indications of a major merger event are apparent, although a mild asymmetry is observed.
