The galaxy presents a mostly smooth, elliptical morphology, with a high degree of central concentration. Its shape is moderately elongated, displaying a subtle cigar-like form. There is a hint of a weak disk structure, however, it is not as well-defined. The light distribution appears relatively uniform, with a gradual decrease in brightness moving outward from the central bulge. There is no evidence of strong spiral arms, dust lanes, or significant star-forming regions. Overall, the galaxy's structure suggests that it is a relatively evolved system, most likely with a limited amount of ongoing star formation activity. There is no strong presence of any interaction or ongoing merger, but there are possible minor disturbances in the edges.
