The galaxy presents as a relatively smooth, elliptical structure with a centrally concentrated, bright core. There appears to be a subtle color gradient visible, with the core exhibiting a yellow-white hue, suggestive of an older stellar population. Fainter, blueish extensions radiate outward from the central region, possibly indicating a population of younger, hotter stars and regions of ongoing star formation. The galaxy appears elongated, with an axis ratio indicating a deviation from perfect circularity. There is an observed morphological disturbance that could be due to a small companion galaxy or a past merger. The galaxy's overall smooth appearance suggests a morphological classification leaning towards an elliptical galaxy, but some features indicate a possibility for more complex star forming regions.