This galaxy appears to be a relatively smooth, early-type system. It exhibits a prominent central bulge, which is significantly brighter and more concentrated than the surrounding disk. The overall shape is elliptical, with a slight elongation. The color gradient suggests an older stellar population, with the bulge displaying a yellowish hue, indicative of evolved stars. The faint outer regions appear somewhat bluer, which could suggest the presence of some younger stars, but overall star formation seems to be relatively quiescent. No distinct spiral arm structures or significant dust lanes are discernible, indicating a lack of ongoing major star formation events or recent merger activity. The galaxy does not display any obvious signs of tidal disturbances or interactions with other galaxies.
