This galaxy exhibits a generally smooth morphology, appearing as an elliptical or lenticular type. It shows a bright, concentrated central bulge that transitions gradually into a more diffuse outer region. The color profile suggests a dominant population of older stars, particularly within the central bulge, implied by the redder hues. Fainter, bluer regions at the edges may indicate some ongoing star formation. There appears to be no strong spiral arm structure or bar feature, and the galaxy shows minimal signs of any major gravitational disturbances or recent merger events. The overall structure appears relatively undisturbed and relaxed.