The galaxy presents as a centrally concentrated object with a roughly elliptical morphology. The light profile appears relatively smooth, suggesting a lack of prominent spiral arms or significant dust lanes. There is a possible slight asymmetry in the outer regions, perhaps indicative of a minor gravitational interaction or tidal disturbance. Color gradients are subtle, with a suggestion of a slightly bluer core compared to the outer regions which are slightly more red, indicating a potential population difference between the central regions and the outskirts. There is no strong evidence of any major ongoing merger events or very significant tidal features. The galaxy is relatively compact in size.
