The galaxy presents as a relatively compact, though not perfectly spherical, object. The central region exhibits a bright, concentrated luminosity, suggesting a prominent galactic nucleus.  The overall color profile leans towards bluer hues in the central region, transitioning to redder tones towards the edges, implying a possible gradient in stellar populations or dust content across the galactic structure. There is an apparent asymmetrical feature or tidal disturbance at the edge of the galaxy, possibly indicative of an ongoing or past interaction with another galaxy or intergalactic material. Further spectral analysis is needed to determine the nature of this structure. The light distribution appears fairly smooth, indicating a lack of prominent spiral arm structures. The galaxy appears to be in an intermediate stage of morphological classification, transitioning between smooth elliptical and more structured spiral types. 
