The galaxy presents as an elongated, cigar-shaped structure. It is characterized by a relatively smooth morphology, with a central bulge that appears more concentrated and brighter than the outer regions. A faint disk-like component is suspected, exhibiting a bluer hue compared to the bulge, suggesting ongoing star formation. The galaxy appears relatively undisturbed, lacking significant signs of recent or ongoing major mergers or tidal interactions. There are no clearly discernible spiral arm structures or prominent dust lanes visible in the image. The light distribution suggests an elliptical or lenticular classification, possibly viewed at a high inclination angle.
