The galaxy presents as an elliptical, or potentially a highly inclined disk galaxy. It displays a generally smooth morphology with no obvious spiral arm structure. The central region exhibits a bright, concentrated bulge which indicates a significant stellar density. The galaxy appears elongated, with a major axis approximately twice the length of the minor axis, suggesting a possible cigar-like shape. Color gradients within the galaxy indicate a bluer core, possibly indicating recent or ongoing star formation, while the outer regions are redder, suggestive of an older stellar population. There are no prominent signs of ongoing mergers or major disturbances, though subtle asymmetries cannot be ruled out at this resolution. The overall appearance suggests a relatively evolved system.
