This galaxy exhibits a generally smooth morphology, suggesting it is likely an elliptical or lenticular type. The central region displays a concentrated luminosity, appearing nearly spherical in shape. The light gradually diffuses outward from the center, with the outer regions appearing less defined. There is a slight elongation present, hinting at a deviation from a perfect spherical form, and no obvious spiral arm structures or dust lanes are visible. The galaxy displays colors leaning towards the redder end of the spectrum, indicating an older stellar population. This observation would be consistent with a passively evolving galaxy, likely with a low rate of ongoing star formation. There is no visual evidence of any major interactions or mergers.
