The galaxy presents as a centrally concentrated object with a relatively smooth morphology. The light profile appears to be largely spheroidal. There is a subtle color gradient apparent, transitioning from a more yellowish hue at the core to slightly bluer tinges in the outer regions. While a distinct disk structure is not readily apparent, there are very faint hints of a possible extension or minor asymmetry, possibly indicating a weak or disrupted disk component, or perhaps an early stage merger. No significant dust lanes are visible, suggesting a lack of significant recent star formation. Given the overall color and structure, this galaxy appears to be an evolved system, likely dominated by an older stellar population.
