The galaxy appears to be a relatively compact elliptical, exhibiting a generally smooth morphology with no obvious spiral arm structures or prominent dust lanes visible at this resolution. The object has a noticeably high degree of central concentration with light appearing brightest at the core, diffusing outwards. The color profile suggests an older stellar population with a redder hue at the center, potentially indicating a concentration of evolved stars. There is a slight asymmetry in the light distribution, possibly suggesting a minor gravitational interaction or an uneven distribution of interstellar material, however no tidal tails are visible. The approximate size of the galaxy is relatively small. Given the overall smoothness and shape of the galaxy, it appears to be in a relatively evolved state.
