The galaxy exhibits an elliptical morphology, appearing as a relatively smooth, flattened spheroid. The galaxy displays a concentrated central bulge which transitions gradually to a diffuse outer halo. The color gradient indicates an older stellar population is dominant. The central region shows a yellowish hue, suggesting a high density of older, cooler stars. A slight blue tinge is seen within the core, which may indicate recent, low levels of star formation in that region. There is no obvious spiral arm structure or significant dust lane visible. There is a slight disturbance detected at the edges, which may indicate a minor interaction. Based on these characteristics, this galaxy is likely a massive, evolved system.
