The galaxy presents a predominantly smooth morphology, appearing somewhat elliptical in shape rather than displaying well-defined spiral arms. The central region exhibits a brighter concentration of light, suggesting the presence of a substantial galactic bulge. The overall color profile indicates a mix of stellar populations, with the central bulge leaning towards a yellow-red hue, potentially indicative of older stars, while the outer regions show a slightly bluer tinge, possibly suggesting ongoing or recent star formation activity. There is a subtle indication of a disk component, but it is not particularly prominent. The galaxy appears relatively isolated with no obvious signs of recent or ongoing major merger events, though there is potentially a minor disturbance. The galaxy is compact in apparent size.
