The galaxy appears to be an elliptical or lenticular type, exhibiting a smooth, largely featureless morphology. The light distribution is centrally concentrated, with a gradual decline in surface brightness towards the outer regions. There is no evidence of spiral arms or a prominent disk structure. The galaxy is nearly symmetrical in shape, with a slight elongation that is visible in this imaging. There is no apparent ongoing major merger or significant tidal disturbance. The galaxy has a yellow-white hue, suggestive of an older stellar population with minimal recent star formation. Overall, it presents as a relatively quiescent system in terms of star formation activity and morphological disturbances.
