The galaxy appears to be a relatively compact elliptical, exhibiting a smooth, featureless morphology. There is no apparent disk structure or spiral arms visible. The light profile is concentrated toward the center, suggesting an older stellar population. The galaxy displays a yellow-orange hue, indicative of evolved stars and a lack of significant ongoing star formation. The roundness is not perfect; it appears slightly elongated. There is no evidence of any major interaction with another galaxy, nor any signs of a strong tidal disturbance or merging event. It is likely a quiescent galaxy that has exhausted much of its gas reservoir.
