The galaxy presents as a smooth, elongated structure, suggesting an elliptical morphology. Its color profile indicates a central concentration of older stars, represented by the yellowish hue. Fainter, bluish regions are observed at the periphery, which could indicate a smaller population of younger, hotter stars or areas of low-level star formation. The overall light distribution appears fairly uniform, devoid of prominent spiral arms or distinct features, consistent with a relatively quiescent stellar population. There is a very slight irregularity on one edge suggesting a possible minor disturbance.
