The galaxy appears as a relatively compact, centrally concentrated object. The light profile suggests a smooth distribution, indicative of an elliptical or lenticular morphology. There is a noticeable color gradient, with the core exhibiting a yellow-red hue that transitions to a slightly bluer color in the outer regions. There is no evidence of strong spiral arms or a prominent disk structure. No significant tidal features or signs of recent major mergers are visible, although a mild asymmetry or minor disturbance cannot be entirely ruled out. The object has a generally elliptical appearance with a relatively rounded shape. Overall, the galaxy's morphology suggests a relatively evolved system with a significant population of older stars.
