The galaxy presents as a smooth, elongated structure, suggestive of an elliptical morphology. The light distribution appears relatively uniform, exhibiting a radial gradient with increased brightness toward the center. The color profile indicates a predominantly red or yellow hue, implying an older stellar population with relatively low ongoing star formation. The galaxy's apparent cigar shape, along with its estimated size, implies that it may be a dwarf galaxy. Based on the lack of any visible signs of disturbance in the image, the galaxy is likely in a relatively quiescent state, undisturbed by major interactions or mergers. 
