The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, diffuse light distribution with no discernible spiral arm structures. Its overall shape is elongated, appearing somewhat cigar-shaped, suggesting a possible E4-E7 classification. The central region displays a concentrated brightness, indicating a prominent galactic nucleus. There is a slight color gradient from the center outwards, with the core appearing more yellowish-orange, transitioning to a bluer hue in the outer regions. This may indicate older stellar populations in the core and younger stars in the outer regions, although the limited resolution makes a definitive assessment difficult. There is a subtle hint of a possible tidal feature or faint extension at one end of the galaxy, however this needs to be confirmed with further investigation. No major distortions or signs of ongoing mergers are immediately apparent.
