The galaxy presents as a relatively smooth, elliptical-like structure, although not perfectly spherical. There is a concentrated central bulge region exhibiting a yellow-white hue, indicative of an older stellar population. Moving outward from the core, the color shifts towards a bluer tint, suggesting the presence of a younger, hotter stellar population, perhaps resulting from ongoing or recent star formation.

There is little evidence of spiral arm structure or well-defined dust lanes. The overall morphology appears largely undisturbed, with no major signs of ongoing merger activity, although a subtle irregularity or minor disturbance cannot be entirely ruled out. The galaxy appears to be fairly massive.
