The galaxy presents as a generally smooth, luminous object with a slightly elongated, elliptical morphology. The central region exhibits a bright, concentrated core suggesting a significant concentration of stars, with the luminosity decreasing towards the outer regions. Color gradients are subtle, but there appears to be a slightly bluer tint near the core region and an overall redder hue in the outer regions. It is difficult to determine the exact morphological type due to the overall smoothness, but it does appear to be undergoing some kind of interaction that is creating disturbed areas. There appears to be evidence of a merging event or tidal interaction with another galaxy, potentially causing disturbances within the system. The redder outer region may indicate an older stellar population. This galaxy exhibits a substantial stellar mass, with relatively low current star formation activity.
