The galaxy presents as a centrally concentrated object, exhibiting a morphology that appears primarily smooth. A slight elongation is discernible, suggesting a possible deviation from a perfectly spherical shape. The core region displays a bright, yellowish hue, likely indicative of an older stellar population. Surrounding this central bulge, a fainter, bluish halo is observed, possibly attributed to younger stars or ongoing star formation activity. The overall color gradient suggests a radial variation in stellar populations, with older stars concentrated towards the center and younger starsPopulations potentiallyPopulations residing in the outer regions. While a dominant spiral structure is not readily apparent, subtle irregularities hint at possible faint features or minor disturbances. There is no strong visual evidence to support a major ongoing merger; however, subtle asymmetry could indicate past interactions or minor accretion events.
