The galaxy presents as a moderately luminous, elongated structure, likely an elliptical or lenticular galaxy viewed at an oblique angle. The core exhibits a concentrated, yellowish hue, indicative of an older stellar population. The outer regions show a gradual decrease in luminosity, with hints of bluer components, potentially suggesting some ongoing, though minimal, star formation within the disk or outer regions. The galaxy appears relatively smooth and undisturbed, showing no strong evidence of recent major mergers or significant tidal interactions. Its overall shape deviates noticeably from a perfect sphere, exhibiting a cigar-like morphology. There are small asymmetries in the outer regions, which might imply minor gravitational disturbances.
