This galaxy presents an elliptical morphology. The object exhibits a smooth, concentrated light profile, suggesting a relatively old stellar population. The color gradient appears to be minimal across the galaxy, with a subtle shift towards redder hues in the central regions, consistent with older stars dominating the core. There is minimal evidence of distinct spiral arms or prominent dust lanes, indicating a lack of significant ongoing star formation. The round shape is evident, with only slight deviations from a perfect circle. There is no visible evidence of any major merging activity. The light output appears relatively consistent across the galaxy, although it does appear to be more compact compared to the other galaxies in the image. 
