The galaxy appears as a moderately bright, centrally concentrated object with a slightly elliptical morphology. The core exhibits a yellowish-white hue, suggesting a population of older stars. A faint disk structure is visible surrounding the core, displaying a bluer color, indicative of more recent star formation. The outer regions of the disk fade gradually into the background, implying a smooth density profile without prominent spiral arms or distinct features. There is no clear evidence of a major ongoing merger, although subtle irregularities in the disk might suggest minor tidal interactions or internal disturbances. Overall, the galaxy presents characteristics consistent with an intermediate-mass system exhibiting a mix of evolved stellar populations and ongoing star formation.
