The galaxy presents a largely smooth, elliptical morphology, exhibiting a concentrated central bulge that dominates the overall light profile. There is a slight elongation along what appears to be its major axis. The galaxy’s core exhibits a yellowish hue, suggesting a population of older stars. Fainter, more diffuse extensions can be observed surrounding the bright central region, implying the presence of a stellar halo or extended outer disk. The galaxy does not exhibit any prominent spiral arm structures or dust lanes. There may be some minor disturbances on the edge of the galaxy, but they are minor. There is an indication of redder color on one side of the galaxy, likely from dust or cooler stars.
