The galaxy appears as a relatively smooth object, exhibiting a centrally concentrated morphology. The light distribution suggests a spheroid-dominated structure, with a subtle color gradient visible. The central region is brighter and slightly redder, indicative of an older stellar population. The outer regions fade into a bluer hue, implying the presence of some younger stars. The galaxy shows little evidence of spiral arm structure or prominent dust lanes. There is no obvious indication of an ongoing major merger event, though subtle disturbances or minor interactions might be present. The galaxy presents as an elliptical galaxy, possibly an intermediate elliptical transitioning from disk galaxy, with a small effective radius.
