The galaxy appears to be a relatively smooth, centrally concentrated system. Its light profile suggests a bulge-dominated morphology, with a possible slight asymmetry. The central region exhibits a yellowish-white color, likely indicating an older stellar population. Fainter, slightly bluer light may exist in the outer regions. There is little evidence of prominent spiral arms or significant dust lanes. There might be very faint disturbances indicating a minor gravitational interaction. The galaxy appears relatively isolated and undisturbed, with no signs of a major ongoing merger.
