This galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The color profile suggests a dominant population of older stars, exhibiting a yellowish-orange hue, implying little ongoing star formation. The galaxy appears to be generally round in shape, with no immediately obvious signs of a prominent disk or spiral arms. There are no strong indications of recent or ongoing major mergers or significant tidal disturbances in its morphology. The galaxy seems fairly isolated, without any close companions significantly disrupting its form.
