The galaxy presents as an elongated, elliptical structure with a smooth overall appearance. Its central region exhibits a concentrated luminosity, appearing bright orange. Fainter, diffuse extensions are visible, suggesting a more extended halo or envelope of stars. The galaxy's shape leans towards a cigar-like morphology, and there are possible signs of minor tidal disturbances or interactions on one side, based on irregular structures observed, but these are not indicative of a major ongoing merger. The dominant color is suggestive of an older stellar population, and there is little evidence of significant ongoing star formation.
