The galaxy presents as a luminous, centrally concentrated object, with an overall smooth appearance. The color profile is predominantly yellow to orange, suggesting an older stellar population and a relatively low rate of ongoing star formation. There are indications of faint, diffuse extensions emanating from the central region; however, there is no clear evidence of spiral arms or a well-defined disk structure. The galaxy does not appear to be undergoing any major merging activity, though minor disturbances cannot be ruled out based on the image alone. Overall, the galaxy appears to be a relatively massive elliptical galaxy with a significant population of evolved stars.
