The galaxy presents a generally smooth, elliptical morphology, appearing largely featureless in this image. The central region exhibits a concentrated, bright core with a yellowish-orange hue, indicating a likely older stellar population. A subtle transition occurs towards the outer regions of the galaxy, which are less luminous and have a slightly bluer tint. The overall round shape suggests minimal rotational support and negligible disk structure. There is a very faint hint of a possible tidal feature or minor disturbance at one end of the galaxy, suggesting a past or ongoing interaction. However, there is no clear evidence of a major merger event or significant star formation occurring within the galaxy's main body.
