The galaxy presents as a relatively smooth, elliptical morphology, with a high degree of central concentration. The color profile suggests a population dominated by older stars, exhibiting a yellowish-red hue. There is no prominent disk structure visible. The galaxy appears to be generally undisturbed, with no obvious signs of recent major merger activity. Faint, diffuse light extends outwards from the central core, suggesting a stellar halo. The round appearance indicates that the object is viewed relatively face-on. There might be a possible, minor disturbance, but not enough to suggest any recent galaxy mergers.
