The galaxy appears to be an elliptical galaxy with a smooth, featureless morphology. The central region exhibits a concentrated, bright core that fades gradually outwards. The overall shape is elongated and cigar shaped. The color profile suggests an older stellar population, with a yellow-orange hue dominating the visual spectrum. There is no apparent evidence of spiral arms, dust lanes, or active star-forming regions. The galaxy appears to be isolated, with no obvious signs of tidal interactions or recent mergers. The galaxy's smooth appearance and color index are consistent with a passively evolving system, suggesting relatively low ongoing star formation.