The galaxy presents a predominantly smooth, elliptical morphology, lacking prominent spiral arms or a well-defined disk structure. The overall light distribution appears centrally concentrated, exhibiting a gradual decrease in brightness from the core outwards. The shape of the galaxy is elongated, suggesting a non-spherical structure, with the major axis oriented at an angle relative to the image frame. There is some evidence of a slight disturbance within the main body of the galaxy, possibly indicating an interaction, or minor merger event. The galaxy's color appears moderately red, hinting at an older stellar population and a relatively low rate of ongoing star formation.
