The galaxy appears to be a relatively compact object. Its morphology is generally smooth, without any obvious spiral arm structure or a prominent disk. The light distribution suggests a spheroidal shape, tending towards round, with a minor elongation observed. There's no apparent strong tidal distortion or indication of a major merger event in progress. Some minor disturbance may be indicated. The central region exhibits a bright, concentrated light profile. The overall color appears relatively blue, possibly indicating the presence of younger stellar populations, though reddening due to redshift must be considered.
