The galaxy appears to be an elliptical galaxy, with a bright central bulge and a fainter, more diffuse halo. The galaxy exhibits an overall smooth morphology, with no apparent spiral arms or disk-like structures. There seems to be minor distortion, possible caused by a merger. The core of the galaxy displays a yellowish hue, suggestive of an older stellar population and reduced star formation activity, while the outer regions show a slight bluer tint, indicating the presence of a younger stellar population. The elongated shape suggests a prolate spheroidal form and some evidence of rotation. The galaxy's redshift indicates that it is a relatively distant object.
