The galaxy presents as an elliptical or lenticular morphology, with a smooth, centralized light distribution. The core region is bright, with an observed color gradient suggesting a possible transition from older stellar populations in the central bulge to potentially younger, bluer stars in the outer regions. The galaxy appears highly elongated, with a major axis significantly larger than its minor axis. There is no evidence of spiral arm structure or significant dust lanes based on the image's resolution and color information, which supports the classification as an elliptical-like galaxy. The color profile indicates moderate levels of star formation. The estimated size indicates the object is a dwarf galaxy.