This galaxy presents as a relatively compact object, exhibiting a smooth, elliptical morphology. The light distribution suggests a high degree of central concentration, with brightness decreasing gradually outward from the core. The galaxy's color index indicates a general lack of recent star formation, evidenced by a dominant population of older, redder stars. While not perfectly spherical, the overall shape is closer to round than highly elongated. There is no obvious evidence of spiral arms, dust lanes, or significant tidal disturbances suggesting it is not undergoing a major merger event, but there is a slight tail to the right of the galaxy that could indicate some form of tidal distruption. Overall, this galaxy appears to be an early-type galaxy which is in the process of being quenched.
