The galaxy presents as a relatively smooth, elliptical-like structure. Its core exhibits a bright, concentrated luminosity, suggesting a high stellar density and potentially a supermassive black hole actively accreting material. The overall color profile leans towards the redder end of the spectrum, indicative of an older stellar population with fewer young, hot stars. There may be a very faint, diffuse disk-like component. The morphology shows no strong indication of a major ongoing merger, although there appears to be some evidence of minor disturbances in the outer regions. The galaxy displays a mostly uniform texture with very little dust.
