The galaxy presents as a relatively smooth, centrally concentrated structure with a slight ellipticity. The core appears as a bright, yellowish-white region, possibly indicative of an older stellar population. The surrounding halo exhibits a bluer hue, suggesting the presence of younger stars or regions of ongoing star formation. There is a slight indication of some disturbance or irregularity in the outer regions of the halo, with a hint of a potential interaction or minor tidal feature. Overall, the galaxy does not show any evidence of a major merger event but may be in the process of a minor interaction.
