This galaxy appears to be a relatively smooth, centrally concentrated system with an elliptical morphology. There is a gradual decrease in luminosity from the core to the outer edges, with no distinct spiral arms or features immediately visible. The color profile suggests a mix of stellar populations, with a slightly bluer hue in the central region, which may indicate ongoing or recent star formation. The overall smoothness suggests a relatively relaxed system, though the slight irregularities in the outer regions may indicate minor disturbances or interactions in its past. This galaxy does not seem to be involved in any major merging activity. The system is moderately sized.