This galaxy appears to be an elliptical type, characterized by a smooth, concentrated distribution of light with no prominent spiral arms or disk structures visible. The galaxy exhibits a yellowish-orange hue, suggestive of an older stellar population dominated by red giant stars. Its overall shape is moderately elongated, falling between a perfectly round and a more cigar-like morphology. There is no evidence of any major mergers or significant tidal disturbances. The light profile gradually fades from a bright central core outwards, indicating a relatively smooth transition in stellar density. Based on the apparent color gradient and lack of distinct features, star formation is likely minimal within this system.
