The galaxy presents an elongated, cigar-shaped morphology, suggestive of an elliptical or lenticular type. The central bulge appears bright and concentrated, exhibiting a yellowish-orange hue, indicating a population of older stars. Surrounding the bulge is a fainter, more diffuse halo extending along the major axis. Hints of blue-green color are observed within the halo, possibly indicating the presence of younger stellar populations or regions of ongoing star formation, although the overall color suggests this is more due to the nature of the image. There is no clear evidence of spiral arm structures or a well-defined disk. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or major mergers.
