The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth, rounded morphology. It shows a relatively concentrated central bulge region with a diffuse, fading halo of light surrounding it. The light is relatively uniform, suggesting an older stellar population. No prominent disk or spiral arm structures are visible. There are only slight hints of possible minor disturbances but overall, the galaxy seems largely undisturbed. The color profile shows a redder hue, consistent with a population of older stars, with a possible active star forming region in the center. 
