The galaxy appears as a centrally concentrated object with a generally smooth morphology. It exhibits a near-spherical shape, appearing mostly round. There is no obvious spiral structure or distinct disk. The galaxy has a bright core region that gradually diffuses outwards. There may be some very faint indication of minor disturbances, though this is within the noise. The color profile indicates a bluer core transitioning to a redder halo, suggesting a possible age gradient in the stellar population. Overall the galaxy seems to have a red shift of about 0.2, estimated size of around 4 kpc, a mass of about 10 to the power of 10 solar masses, with a small rate of star formation.
