The galaxy in question appears as a relatively compact, luminous object. Its overall color profile indicates a spectral shift towards the redder end of the spectrum. The morphology is predominantly smooth, with only subtle features that suggest some minor internal structure. The galaxy has an apparent size of approximately 2 arcseconds and has an approximate distance of 9.5 kpc. The general appearance points to a relatively evolved system, with a significant stellar mass. There is some visual evidence of minor disturbances, possibly resulting from a past interaction or internal dynamical processes. This does not appear to be a major merger event. It displays a moderate rate of star formation and has a high mass. Its rounded shape is more of an intermediate nature than a distinctly round or elongated appearance.
