The galaxy appears to be an elliptical or lenticular type, exhibiting a smooth, concentrated luminosity profile. It displays a pronounced elongation, suggesting a cigar-like shape rather than a perfectly circular structure. The central bulge is a bright yellow-orange color, indicating a concentration of older stellar populations. The outer regions show a gradual fading of luminosity, appearing somewhat bluer, possibly due to a small amount of younger star formation but this effect is very minimal. There is no evidence of spiral arms or significant dust lanes. The overall structure suggests a relatively evolved system, with ongoing, but low star formation. The galaxy appears isolated with no signs of interaction.
