The galaxy presents a predominantly smooth morphology, with a relatively high degree of central concentration. Its apparent shape is somewhat elongated, displaying an aspect ratio that deviates moderately from perfect circularity. There is a faint suggestion of a disk component or some other distinct structural feature, although the overall smoothness of the galaxy dominates its appearance. The galaxy's color gradient suggests a possible cessation of star formation in the central regions, as its core seems to be more red compared to the outer regions. Furthermore, there is the distinct possibility of tidal disturbance due to the slightly irregular shape. Signs suggest that the galaxy is merging with another galaxy, or has in the recent past. This galaxy has a high mass and it is likely to be dominated by older stars.
