The galaxy presents as a centrally concentrated spheroid, exhibiting a largely smooth morphology. There is no prominent disk structure discernible, nor are there any obvious spiral arms. The central region displays a reddish hue, potentially indicative of an older stellar population. Surrounding the core is a more diffuse, greenish halo. The overall shape of the galaxy is generally round, with no significant elongation or tidal features observed, suggesting it is likely not undergoing a major merger. There are no prominent dust lanes or regions of active star formation immediately visible in this image, based on its smooth texture and color profile.