The galaxy presents as a centrally concentrated object, exhibiting an elliptical morphology with a moderate axial ratio. There is evidence of a smooth luminosity profile, indicating a relatively homogenous stellar population. The galactic center is characterized by a brighter, more condensed region, likely containing a supermassive black hole. Extending outwards from the core, there is a diffuse halo with a slightly irregular shape, possibly indicating past minor interactions or mergers. The galaxy appears to have a generally blue color, suggesting the presence of young, hot stars undergoing active star formation. However, the concentration of light towards the core suggests an older, more evolved population may dominate the central regions. Overall, the galaxy shows a mix of features indicative of both ongoing star formation and a more quiescent, evolved stellar population. The overall structure appears relatively undisturbed, without the pronounced tidal tails or distorted morphologies associated with major mergers.
