The galaxy presents as a somewhat compact object, exhibiting a roughly elliptical morphology. The light distribution appears relatively smooth, with a slightly brighter central region. Faint hints of asymmetry are present, but no clearly defined spiral arms or a distinct disk component are readily discernible. The overall color gradient suggests the presence of a mixture of stellar populations, with the inner region potentially hosting older, redder stars while the outer regions may have a contribution from younger, bluer stars. There are no strong signs of a major ongoing merger, but some minor disturbances cannot be excluded based on the morphology. The galaxy's general appearance indicates it is likely an intermediate-redshift object.
