This galaxy appears as a luminous, centrally concentrated object. It has a smooth morphology, with a largely elliptical shape, and it is relatively rounded. There is some indication of a slight disk-like structure; however, any disc features are faint. There is no evidence of significant spiral arm structure or strong dust lanes within the resolution of this image. The galaxy exhibits a color gradient, trending toward redder hues near the core. This suggests an older stellar population is dominating the central regions. There does not appear to be significant evidence of ongoing major merging events.
