The galaxy presents as an elliptical morphology, appearing largely smooth and featureless. A concentrated central bulge dominates the overall structure, exhibiting a bright, yellowish hue. The light profile diminishes gradually outward from the core, suggesting a lack of significant ongoing star formation in the outer regions. There is an absence of spiral arms or a well-defined disk structure, supporting the classification as an elliptical galaxy. The overall shape is tending towards round, with no apparent tidal disturbances or signs of recent merger activity. The color indices suggest the presence of an older stellar population.
