The galaxy presents as a centrally concentrated object with a relatively smooth overall appearance. The central region exhibits a noticeable red color, suggesting an older stellar population, and a considerable mass. The galaxy is somewhat cigar shaped, showing a very faint disk like structure and is likely not undergoing a major merger, as it doesn't show substantial signs of ongoing tidal disruption. The faintness of the disk like structure suggests a low star formation rate within the galaxy, further supported by the dominant red color.
