The galaxy presents as a relatively smooth, elliptical-like structure, appearing elongated with a cigar-shaped morphology. The light distribution is centrally concentrated, exhibiting a bright, yellowish core that fades gradually towards the outer regions. There's minimal evidence of distinct spiral arms or prominent dust lanes. The overall color suggests a population of older stars, consistent with a relatively low star formation rate. Some minor visual disturbance is present, with no clear signs of a major merging event. 
