This galaxy presents as a disk-dominated system, but with some features of an elliptical galaxy. The central bulge is prominent but appears somewhat obscured, possibly due to dust or gas. Faint spiral arms are tentatively observed extending from the bulge, indicative of ongoing, albeit weak, star formation. The overall color suggests a moderate population of older stars, as well as some younger, bluer stars within the spiral arms. The galaxy exhibits a relatively smooth appearance, although a minor asymmetry or disturbance is noted in its morphology, hinting at a possible interaction or past merger event. The galaxy's shape appears to be of an intermediate form, displaying a round shape that does not fit strictly into an elliptical or spiral category.
