The galaxy presents as an elliptical morphology, exhibiting a largely smooth and centrally concentrated light distribution. The core of the galaxy appears bright and unresolved, characterized by a yellowish hue suggesting an older stellar population. The light profile gradually decreases with radial distance from the core. The outer regions of the galaxy are less distinct and appear more diffuse. There is no evidence of prominent spiral arms, dust lanes, or other significant features indicative of recent star formation. Overall, the galaxy's appearance suggests a quiescent system dominated by an older stellar population.
