This galaxy presents an elliptical morphology. A bright, concentrated nucleus is observed, surrounded by a fainter, diffuse halo. The halo exhibits a generally smooth texture, with a slight flattening along the major axis. Visual assessment suggests the galaxy is generally undisturbed with no significant tidal tails or distortions. The galaxy's color profile indicates a relatively uniform distribution, with slightly redder hues concentrated on the outer edges of the halo. No distinct spiral arm structures or prominent dust lanes are discernible, indicating a more evolved system with less ongoing star formation. There is a slight hint of a disturbance, most likely in the form of minor merger with another galaxy, but without further information such as redshift, it is hard to determine what is affecting the galaxy. 
