The object presents as a lenticular galaxy with a smooth, elongated profile. Its color gradient transitions from a yellowish core towards a bluer, diffuse outer region. The central bulge dominates the galaxy's luminosity, indicating a significant population of older stars. The disk is not well-defined, lacking prominent spiral arms. A slight warp or tidal feature may be present in the outer regions but does not suggest a major merger event. There is no visual evidence of active star formation in the core. The overall morphology suggests an evolved system with a moderate mass, perhaps undergoing slow, ongoing star formation in the outer regions of the disk.
