The galaxy appears as a relatively smooth, centrally concentrated object. Its shape is neither perfectly spherical nor highly elongated, presenting an intermediate, elliptical appearance.

The galaxy exhibits a color gradient, with a slightly redder core transitioning to bluer outer regions. This suggests possible variations in stellar populations, with older, redder stars concentrated towards the center, and younger, bluer stars more prevalent in the outer regions.

There is no discernible spiral structure or prominent dust lanes visible. The galaxy appears largely undisturbed, with no clear evidence of recent major merger events, although subtle disturbances cannot be ruled out.
