The galaxy presents an overall smooth morphology, with a centrally concentrated light profile. It appears elliptical in shape, exhibiting a slight elongation. The core region is bright and concentrated, suggesting a possible bulge component. The galaxy's color gradient indicates a redder population in the central regions, possibly indicating older stars. Fainter, bluer light extends outward along the disk-like structure, which suggests more recent star formation is occuring within the galaxy. There are no readily apparent signs of any major disturbances or interactions with other galaxies, indicating a relative state of isolation.
