The galaxy presents an overall elliptical morphology, appearing generally smooth in texture with a slight elongation. The core region is notably bright, exhibiting a yellowish hue, suggestive of an older stellar population. There is a faint, smaller region close to the core that exhibits a bluer tint, hinting at the presence of younger, hotter stars or ongoing star formation. The galaxy shows some evidence of disturbance, possibly the result of a past or ongoing interaction with another galaxy, especially towards the northern portion. There are no distinct spiral arms or a well-defined disk structure visible. The overall color profile indicates a significant population of evolved stars, although the localized blue region suggests ongoing stellar activity.
