The galaxy presents as a relatively smooth and elliptical structure. The core appears centrally concentrated with a yellowish hue, suggestive of an older stellar population. The disk exhibits a bluer color gradient extending outwards from the core. The disk does not display prominent spiral arm structures. The galaxy appears elongated, indicating a non-spherical shape. The outer edges are fairly uniform and do not show signs of significant tidal disturbances or ongoing major mergers. There are no obvious dust lanes visible. Based on the overall morphology, this galaxy can be described as an intermediate elliptical-to-spiral galaxy.
