The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and concentrated light distribution. It is moderately elongated, with a cigar-like shape. The central region is bright and yellowish, suggesting a population of older stars. There is little evidence of spiral arms or significant dust lanes. The galaxy exhibits a slight blue tinge in the outer edges, indicating a younger stellar population in these regions, possibly a remnant of past star forming activity. No significant tidal tails or merger signatures are visible, implying that the galaxy has not recently undergone a major merger event. Any perturbations are minor. The overall appearance suggests a relatively evolved galaxy with a dominant spheroidal component.
