The galaxy presents as a smooth, elliptical form, exhibiting a concentrated central bulge. The light distribution appears largely uniform, with a radial gradient decreasing from the core outwards. The color profile is predominantly reddish-yellow, suggesting an older stellar population and lower rates of ongoing star formation. There is subtle indication of a faint, diffuse halo extending beyond the main body of the galaxy. The object does not exhibit any obvious spiral arm structure or significant dust lane features. There is some indication of minor irregularities which could be from minor gravitational disturbances, but overall the galaxy appears to be relatively undisturbed.
