The galaxy appears to be an elliptical or lenticular type, exhibiting a predominantly smooth morphology. A disk component is not readily apparent. The light distribution appears centrally concentrated, gradually fading towards the outer regions. It presents an intermediate ellipticity, not perfectly spherical but also lacking a highly elongated, cigar-like shape. The overall structure suggests that the galaxy is likely isolated with no immediate indications of a major merger event or significant tidal disturbances. Faint features might exist, but they are difficult to resolve.
