The galaxy presents a morphology consistent with an elliptical galaxy or a spheroid-dominated system. It exhibits a generally smooth light distribution, though with possible disturbances or mergers occurring. The galaxy has a concentrated central region with a gradual decrease in luminosity towards the outer regions. There is at least one distinct bright region or core, with another secondary region close by, suggesting a dual core possibly formed from a merger event. The color gradient shifts from a bluer hue in the core to redder hues in the extended regions. The galaxy appears relatively compact, with an estimated effective radius of approximately 5.8 kpc. The visual color, being relatively red, suggests a stellar population dominated by older, evolved stars, consistent with a relatively low ongoing star formation rate. There are some signs of tidal disruption or interaction.
