The galaxy presents as a centrally concentrated, smooth structure with a notable lack of distinct features such as spiral arms or prominent dust lanes. The overall morphology appears relatively round, with a slight deviation towards an intermediate shape. There is no indication of a major merger event, though subtle disturbances or asymmetries cannot be entirely ruled out. The color profile suggests a population dominated by older stars, with a redder hue in the central regions, hinting at a suppressed rate of star formation. The galaxy exhibits a moderate luminosity.
