The galaxy presents a primarily smooth morphology, with a highly concentrated central bulge. The galaxy appears to have a roughly elliptical shape, showing minimal disk-like features or spiral arm structures. The color profile suggests a dominant population of older stars, with a bias towards redder wavelengths across the galaxy's visible extent. There is little evidence of significant ongoing star formation in this image. While the core is very bright, there may be some interaction occurring giving rise to a merger like disturbance on the outer edges of this galaxy.