The galaxy presents as a relatively smooth, concentrated object with a roughly elliptical morphology. The central region exhibits a bright, yellowish hue, suggestive of an older stellar population, where star formation may be suppressed. This core blends into a fainter, bluer disk structure, indicating the presence of younger stars, and possibly ongoing star formation. There are no immediately obvious signs of spiral arms or a central bar. The galaxy appears undisturbed, showing no major tidal features or signs of a recent merger event.
