The galaxy presents as a relatively smooth, elliptical morphology. Its core exhibits a concentrated luminosity gradient, appearing bright and somewhat golden in color, indicative of a population of older stars. Faint extensions appear on either side of the bright core, suggesting a slightly elongated shape. No distinct spiral arms, dust lanes, or other prominent features are readily discernible in the image. The overall color suggests a quiescent or passively evolving system, with a low rate of ongoing star formation. There is no visible evidence of any major merger events or tidal disturbances affecting its structure, although some minor disturbances can not be ruled out.
