The galaxy presents as an elliptical or lenticular type, characterized by a relatively smooth and featureless morphology. There is no prominent spiral arm structure or dust lane visible. The light distribution suggests a centrally concentrated bulge, with the intensity gradually decreasing outwards.

The color profile indicates a population of primarily older stars, exhibiting a yellowish hue in the central region. Faint bluish extensions on the outermost edges suggest the presence of a small number of younger, hotter stars or ongoing low-level star formation in the outskirts. The galaxy appears slightly elongated, with a cigar-like shape, and shows no obvious signs of major mergers or significant tidal disturbances.
