The galaxy presents as a centrally concentrated elliptical or lenticular type, exhibiting a smooth, diffuse morphology. Its color profile is relatively uniform, with a yellowish hue suggesting an older stellar population. The absence of prominent spiral arms or dust lanes indicates a lack of significant ongoing star formation. There's no apparent disruption or tidal features, suggesting it is not currently undergoing a major merging event. Overall, the galaxy appears to be a relatively quiescent system.
