The galaxy presents as an elliptical morphology with a smooth, centralized light distribution. The core region exhibits a bright, concentrated luminosity profile. Faint color gradients are potentially visible across the galaxy, transitioning from a slightly bluer hue in the outer regions to a redder, more yellow tint toward the nucleus. The overall shape is predominantly round. There is no clear evidence of spiral arms or other distinct features. A faint halo may be present, though difficult to discern due to image limitations. No significant signs of tidal disturbances or ongoing major merging activity are readily apparent. The object displays a color index suggesting a population of older stars and a relatively low current rate of star formation.
