The galaxy presents as a relatively smooth, elliptical-like structure. The light distribution suggests a prominent central bulge, characterized by a high concentration of older stellar populations, with an overall yellowish hue. The isophotes exhibit a moderate ellipticity. A disk component may exist but is not as evident, but it does appear that bluer colors start to come into play on the edges of the galaxy, implying at least some lower levels of star formation. There is no obvious strong tidal distortion or evidence of a recent major merger event in the image. However, there might be a faint indication of a minor interaction or internal disturbance within the galaxy, as the image is not perfectly symmetrical.
