The galaxy appears to be an elliptical type, with a predominantly smooth and centrally concentrated light distribution. A subtle disk-like feature may be present, though the overall structure lacks well-defined spiral arms. There is a noticeable tidal tail extending from one side of the galaxy, indicative of gravitational interaction. This suggests a possible merger event, which is also supported by the observed disruption in the overall galaxy shape. The galaxy exhibits a range of colors across its body, suggesting a range of stellar populations.
