This galaxy presents as a single, fairly smooth structure with hints of a possible close companion. The primary body exhibits a concentrated central bulge with a yellowish hue, suggesting an older stellar population likely dominating its composition. Moving outward from the core, there is a subtle decrease in luminosity, implying a radial decline in stellar density. The overall form is relatively round, indicating a potential elliptical morphology or a spiral galaxy viewed at a high inclination. A minor disruption in the upper region exhibits a slightly bluer color, and is less concentrated, suggesting a possible region of ongoing star formation. This could be a result of interaction with the possible companion galaxy, which appears to be an area of lower density than the central region. There may be indications of past or current interaction in the form of minor tidal features or distortions. Further investigation is necessary to clarify the exact nature of this interaction and its impact on the evolution of the central galaxy.
