The galaxy appears as a centrally concentrated object with a generally smooth morphology. There's a noticeable radial gradient in luminosity, with a bright, almost stellar-like core fading into a diffuse halo. The overall shape appears to be roughly elliptical, tending toward circular. The color profile suggests an older stellar population, appearing somewhat redder towards the central region. There is a hint of bluer color in the surrounding halo, potentially indicating recent star formation, however, no distinct spiral arm structure or prominent dust lanes are discernible. There are no signs of any major ongoing merger events, although some minor disturbances cannot be ruled out due to the limited resolution. The object appears relatively isolated and undisturbed within its immediate environment.
