The galaxy presents as a somewhat smooth, elliptical-like structure. It exhibits a centrally concentrated light profile, with the highest intensity emanating from the core region. There is a diffuse, fainter halo surrounding the core, gradually fading into the background.  The overall shape appears relatively round, with no significant elongation or asymmetry readily apparent.  While appearing primarily smooth, there are hints of subtle, faint features within the extended halo that could indicate minor disturbances, but these are not pronounced. The color appears to be on the bluer side, which suggests the possible presence of younger stars, though this may be offset by the overall red shift and the age of the object.  There is no indication of a prominent disk structure or spiral arms from the image. Overall, the galaxy morphology points to a system that has largely settled, with a moderate stellar mass and a low but measurable star formation rate.
