The galaxy exhibits a generally smooth and rounded morphology. There is a strong central bulge, brighter in the green and red bands than in the blue, which diminishes in intensity with radial distance. The overall shape is elliptical, displaying a slight elongation without any obvious spiral arm structures or significant dust lanes. Minor disturbances are possibly present, but the galaxy is mostly undisturbed. The color profile suggests an older stellar population, with a moderate redshift consistent with its estimated distance. There is no clear evidence of ongoing major star formation activity. The galaxy does not appear to be actively merging with another galaxy. The observed structure indicates a likely early-type galaxy, possibly an elliptical galaxy.