The galaxy presents a somewhat amorphous structure, exhibiting characteristics that suggest it may be undergoing or have recently undergone a merging event. It appears to be an intermediate galaxy in morphology, showing features of both smooth elliptical galaxies and galaxies with disks and complex structures. There is a notable central bulge, slightly elongated, displaying a yellow-reddish hue suggestive of an older stellar population. Fainter, diffuse outer regions surround the core, with a greenish tint hinting at possible ongoing star formation or younger stellar populations in these areas. The overall luminosity profile seems to gradually fade outwards from the central region without any distinct spiral arm structure, consistent with the classification of an early to intermediate type galaxy experiencing some level of disturbance.
