The galaxy presents as a centrally concentrated, elongated structure. It exhibits a smooth, lenticular morphology, with a notable absence of distinct spiral arms or prominent dust lanes. The color profile suggests an older stellar population, with a yellowish-red hue dominating, particularly in the central bulge. The outer regions of the galaxy appear fainter and bluer in color. This color variation indicates that the center is mostly older stars while the outer reaches show areas of younger star formation. There is no apparent significant tidal disturbance or interaction with nearby galaxies, and the overall symmetry suggests a relaxed system, post-merger.
