The galaxy appears as a relatively small, centrally concentrated object. It exhibits a generally smooth morphology. A notable feature is the apparent roundness of the object. There are no clear spiral arm structures or distinct bar features. It exhibits a centrally concentrated luminosity profile and a lack of significant disturbances or merging features, suggesting that it is a relatively isolated and unperturbed system. The galaxy shows no strong indicators of recent major merger activity or tidal interactions. The galaxy's color suggests relatively older stellar populations, with a subtle shift towards redder wavelengths. Overall, the galaxy appears to be a relatively quiescent, possibly elliptical system with a lack of significant ongoing star formation.