The galaxy presents as a slightly elongated, lenticular-like structure. Its central bulge is prominent, exhibiting a smooth, diffuse glow, indicative of an older stellar population. Extending outward from the core, a faint disk is subtly visible, though largely featureless in this observation, with what may be faint spiral arms visible. There is little evidence of ongoing, intense star formation. The galaxy is moderately large and massive. It is likely experiencing a low rate of star formation. The overall structure suggests a galaxy that is evolving towards a more quiescent state. There is indication of only minor interactions or disturbances affecting the galaxy's morphology. The galaxy is mostly between a round and cigar shape. 
