The galaxy presents as a smooth, elliptical morphology. It exhibits a notable central bulge characterized by a higher concentration of light, suggesting a greater density of stars in the core region. The galaxy appears elongated, with an approximate axis ratio suggesting it is more cigar-shaped than circular. Little to no distinct disk structure or spiral arms are visible. The overall color profile leans towards redder hues, with diminishing blue components in the outer regions. This color gradient may indicate an older stellar population with ongoing star formation concentrated more centrally, at a relatively low rate. There is no readily apparent evidence of major mergers or significant tidal disturbances. Minor perturbations cannot be ruled out, but they are not immediately discernible from the image. The galaxy’s size appears relatively compact.
