The galaxy presents as a centrally concentrated object with a generally smooth morphology. It exhibits a roughly elliptical shape, appearing mostly round rather than elongated. The core is a bright, yellowish hue, suggesting an older stellar population. The galaxy gradually fades from its core. Faint traces of what may be spiral structures are barely visible in the disk. There is no obvious evidence of ongoing major mergers or tidal disruptions, however, a minor disturbance in the galaxy shape is possible. The galaxy has a redshift indicating it is a distant object. Given its apparent size, the physical extent is significant.
