The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated luminosity profile. The galaxy exhibits an overall color gradient transitioning from a bluer, possibly star-forming region in the core to a redder halo. The object's shape is more in-between round and cigar shaped. The observed light suggests a evolved stellar population, potentially with lower levels of recent star formation. There is no apparent interaction or major disturbance within the galaxy's structure. The object appears isolated in this field of view.
