This galaxy exhibits a generally smooth morphology. It appears largely elliptical, though not perfectly so, with a deviation towards a more intermediate shape. The galaxy demonstrates a notable concentration of light towards the center, suggesting a prominent bulge. Faint, diffuse extensions can be observed emanating from the central region, hinting at a possible disk component or tidal features, but they are poorly defined. The color profile indicates a redder central bulge transitioning to bluer outer regions. There is no strong evidence of ongoing major merging activity, although minor disturbances cannot be ruled out. Star formation appears relatively subdued based on the overall color and lack of prominent blue knots or HII regions. The galaxy's estimated mass is substantial.
