This galaxy presents a primarily smooth morphology, suggestive of an elliptical or lenticular classification. Its shape appears elongated, exhibiting a cigar-like form. The light distribution is concentrated in the center, indicative of a prominent bulge. The color profile suggests an older stellar population, with redder hues dominating the central regions and slightly bluer tinges towards the outer edges. There is no clear evidence of spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, lacking any obvious signs of a recent or ongoing major merger event. Faint asymmetric features could imply a past minor interaction. Star formation is present, but at a subdued rate, indicated by the subtle bluer colors in the disk.
