The galaxy presents an elliptical morphology, appearing largely smooth and with a high degree of central concentration. The light profile appears somewhat regular, lacking prominent spiral arms or distinct features. The galaxy exhibits a moderate level of elongation, deviating slightly from a perfectly circular shape. The color profile shows a shift towards redder hues in the central regions, suggestive of an older stellar population dominating the core. Some bluer light is present, indicating some recent star formation activity. There are no immediately apparent signs of major mergers, though the overall morphology is somewhat disturbed, and does suggest a potential recent or ongoing minor interaction or disturbance. The galaxy appears as a singular entity within its immediate surrounding space, without clear indicators of tidal tails or streams.