The galaxy presents a generally smooth, elliptical morphology. The light distribution suggests a central bulge that is approximately spherical, surrounded by a more diffuse halo. There is little evidence of spiral arm structure or prominent dust lanes. The color profile appears relatively uniform across the galaxy, indicating a possibly older stellar population. There's a lack of any noticeable tidal features or morphological disturbances, indicating that the galaxy has likely not undergone a major merging event recently.
