The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, appearing yellowish-white, suggesting a population of older stars. The overall shape is somewhat elongated but not significantly cigar-shaped; the galaxy appears to be somewhere in between circular and elongated. There are hints of faint, diffuse, greenish-blue emission surrounding the central region, potentially indicating some ongoing, but very low, star formation. There is no strong evidence of spiral arms or a well-defined disk. There are no signs of ongoing major mergers or significant tidal disturbances in the immediate vicinity of the galaxy, although subtle minor disturbances cannot be ruled out. The galaxy’s color profile suggests a redder overall stellar population consistent with a galaxy at moderate redshift.
