The galaxy appears to be an elliptical galaxy, characterized by a generally smooth and rounded morphology. There are no distinct spiral arms or bar structures visible. The central region exhibits a concentrated brightness, indicating a dense stellar population, with an apparent decline in stellar density moving outwards toward the edge. There are tinges of red in the color profile. The overall color index suggests a population of older stars, and low ongoing star formation activity, consistent with an elliptical classification. The galaxy may be undergoing a minor merger based on slight irregularities in its outer shape.
