The galaxy appears to be an elliptical or lenticular type, exhibiting a relatively smooth and featureless morphology. There is a concentrated central bulge that dominates the galaxy's luminosity. A faint, extended halo is visible surrounding the central region, gradually fading into the background. The galaxy displays a slightly elongated shape. Some irregular features may be indicative of minor tidal disturbances or ongoing mergers. Overall, the galaxy appears as a evolved, relatively quiescent system with little evidence of active star formation. The color profile suggests a population of older stars.
