The galaxy appears to be a relatively smooth, rounded object with a concentrated central bulge. The color distribution suggests a higher concentration of older stars toward the center, indicated by the slightly redder hue in the bulge region. Moving outwards, the galaxy gradually transitions to a bluer color, suggesting a younger stellar population in the outer regions. There is no discernible spiral structure or significant dust lanes. There are some subtle hints of minor disturbances in the outer halo, potentially indicating a past or ongoing minor merger event. The galaxy presents as a relatively undisturbed, mature system, likely an elliptical or S0 type. Its estimated size is approximately 3.6 kpc.