The galaxy presents a centrally concentrated light profile, indicative of a dominant bulge component. Its overall structure is generally smooth. There is a hint of disk-like structure, but it is not well-defined. The galaxy's shape is largely round, with a very slight deviation towards an elongated form. There is no clear indication of ongoing major merger activity or significant tidal disturbances. The color gradients suggest that the inner regions are redder compared to the outer areas, possibly indicating a gradient in stellar population age or dust content. Overall, this appears to be a moderately massive galaxy.
