The galaxy presents a relatively smooth and symmetrical morphology, consistent with an elliptical or lenticular classification. The light distribution appears concentrated towards the center, indicating a prominent bulge component. There is a faint suggestion of a disk-like structure viewed edge-on, but it is not well-defined. The galaxy is relatively isolated, showing no immediate signs of tidal interactions or ongoing mergers. Its color profile suggests a population dominated by older stars, with only subtle variations in color across its structure. The galaxy exhibits an overall red hue, indicative of evolved stellar populations and minimal active star formation. There is no apparent dust lane or significant morphological peculiarities.