This galaxy presents as a moderately bright, centrally concentrated object. The core exhibits a smooth, yellowish-orange hue, suggesting an older stellar population dominating the central region. Moving outwards from the core, a subtle gradient transitions to a slightly bluer periphery. The galaxy lacks any distinct spiral arm structure or prominent dust lanes visible at this resolution. The overall shape appears largely elliptical or spheroidal, exhibiting high degree of roundness. There is no compelling evidence of any major ongoing merger events or significant tidal disturbances, although some minor asymmetries cannot be entirely ruled out. The galaxy appears relatively isolated and well-defined.
