The galaxy appears as a relatively compact and faint object. Its morphology is generally smooth, exhibiting a centrally concentrated light profile. There is a slight elongation and asymmetry, suggestive of an elliptical morphology, but there is no strong evidence of spiral arms or a distinct disk structure. The galaxy does not appear to be actively merging, but there is a minor likelihood of a past disturbance that may be slightly influencing its present shape, but I cannot confirm. The galaxy is likely to be quite massive, with correspondingly low specific star formation, as this is consistent with the older stellar populations that comprise the light emitted in g, r, and z bands. I estimate that this object has a diameter of around 7 kpc. The roundness of the galaxy appears to be in between round and cigar-shaped, but I cannot confirm if this is entirely influenced by a past disturbance.
