The galaxy presents as a slightly elongated, centrally concentrated luminous object. It appears to possess a smooth morphology, with no readily discernible spiral arms or distinct features. The central region exhibits a yellowish hue, possibly indicative of an older stellar population. The outer regions fade in intensity, displaying a subtle blueish tint, which could suggest the presence of younger, hotter stars, or ongoing star formation activity within the galaxy's disk. There is no apparent evidence of significant tidal disturbances, major mergers, or other strong gravitational interactions.
