The galaxy appears as a relatively smooth, centrally concentrated object. It is generally elliptical in shape, displaying a high degree of roundness with no discernible spiral arms or bar structures. There is a smooth, gradual decline in luminosity from the center outwards with some minor patchiness in brightness across the galaxy’s extent.

The color profile suggests a population dominated by older stars, exhibiting a reddish hue indicative of a lack of significant ongoing star formation. There is no evidence of dust lanes or tidal features indicative of recent mergers. The galaxy appears to be relatively undisturbed, showing a classical elliptical morphology with no major structural distortions.
