The galaxy presents as a somewhat elliptical structure with a relatively smooth, centrally concentrated light distribution. The core region appears bright, possibly indicative of an older stellar population. Fainter extensions emanate from the central region, contributing to the overall elliptical shape. There is a slight asymmetry in the light distribution, potentially pointing to past interactions. The galaxy exhibits a reddish hue, consistent with a galaxy at its redshift. There may be ongoing but minimal star formation.
