The galaxy presents as a somewhat featureless, centrally concentrated object. It appears to exhibit a spheroidal morphology, lacking any obvious spiral arm structures or a distinct disk component. The central region displays a bright, concentrated core, possibly indicative of an active galactic nucleus or a dense stellar population. The color profile suggests a generally older stellar population, with a subtle shift towards redder hues, though there's a hint of blue in the outer regions implying some recent star formation. The galaxy seems relatively isolated, displaying only minor disturbances in its overall form, potentially hinting at past interactions or minor merging events. The galaxy's shape is moderately rounded, and the size is relatively compact.
