The galaxy presents an overall elliptical morphology, with a noticeable asymmetry in its structure. One side of the galaxy exhibits a smooth, concentrated bulge, characterized by a yellowish-orange hue, suggesting an older stellar population with lower levels of ongoing star formation. Conversely, the opposite side reveals a diffuse, bluish region, indicative of more recent or active star formation. The galaxy is not perfectly round, showing an elongated appearance with a slightly disturbed shape. There may be a minor interaction or internal dynamic process causing the observed morphological distortion. Evidence of merging or tidal features is present, with noticeable disturbances.