This galaxy presents a smooth, elliptical morphology. It appears largely featureless with a high degree of central concentration, exhibiting a bright, well-defined core that gradually fades into its outer regions. The galaxy's light profile suggests a relatively even distribution of older stars with little evidence of significant dust lanes or spiral arm structures. There's a slight elongation in its shape, indicating a degree of flattening rather than perfect sphericity. The color indices suggest a redder overall population, consistent with an older stellar population and a lower rate of ongoing star formation.
