The galaxy presents as a slightly elongated, centrally concentrated object. Its light profile appears relatively smooth, with a noticeable lack of distinct spiral arms or prominent features indicative of active star formation regions. The color gradient shifts subtly from a yellowish-white core to bluish hues towards the outer edges. This may suggest a difference in stellar populations, with older, redder stars concentrated in the center and younger, bluer stars being more common in the periphery. The overall structure appears relatively undisturbed, with no obvious signs of recent mergers or major tidal interactions. There is a slight asymmetry in the shape, potentially indicating a minor interaction or internal dynamical process.
