The galaxy presents as an elliptical or lenticular system, exhibiting a smooth, diffuse light profile with no readily discernible spiral arm structure. The central bulge appears bright and concentrated, suggesting a significant population of older stars. The isophotes of the galaxy appear elongated, hinting at a possible cigar shape.  There is no evidence of strong tidal features or ongoing major mergers. The galaxy appears to be in a relatively quiescent state, showing limited signs of recent star formation. A faint, extended halo may surround the main body of the galaxy.
