The galaxy presents as an elliptical morphology, exhibiting a smooth, diffused light profile. There's a noticeable concentration of luminosity towards the galactic center, which appears bright and slightly yellow-shifted compared to the outer regions. The overall shape is somewhat elongated, displaying a cigar-like form, with no immediately apparent spiral arms or distinct disk structures. There might be subtle disturbances present, though a major ongoing merger is unlikely. The galaxy's color suggests a population of older stars, implying relatively low current star formation activity.
