The galaxy presents as a centrally concentrated, smooth object with an elliptical morphology. The color gradient suggests a dominant stellar population with older, redder stars concentrated towards the center. There appears to be a very subtle, fainter, and bluer disc component. No distinct spiral arms or prominent dust lanes are visible. The overall light distribution is relatively even and lacks any significant morphological disturbances, suggesting it is likely not undergoing a major merger event. The galaxy appears well-defined, indicating a stable structure.
