The galaxy presents as a relatively smooth, elliptical or lenticular type. It exhibits a subtle central concentration of light, with luminosity decreasing gradually towards the outer edges. The morphology is generally smooth and lacks prominent spiral arm structures or significant dust lanes. There is a slight elongation, with an axial ratio suggesting it is somewhat cigar-shaped rather than perfectly circular. Overall, the galaxy appears relatively undisturbed, showing no strong signs of a recent major merger or tidal interactions. The color profile indicates a possible presence of older stellar populations, with subtle color variations, although the image resolution limits a detailed analysis of the stellar populations. There are no prominent active galactic nuclei features visible. The light emitted suggests a low star formation rate. The galaxy appears to be a mature system.
