The galaxy presents as a moderately bright, elongated spheroid. It displays a prominent, concentrated core region, with a visible radial decrease in luminosity moving outwards from the center. The light profile suggests a relatively smooth distribution, with some subtle irregularities. There is evidence of a disk structure, but it's less prominent. The galaxy has a slight cigar shape.  Its color index indicates a possible intermediate-age stellar population, with hints of active star formation. A possible minor disturbance is present, suggesting a recent or ongoing interaction. There are no indications of a major merger. 
