This galaxy presents a moderately elliptical morphology. Its core exhibits a bright, concentrated luminosity, suggesting a substantial stellar population. The galaxy appears to be relatively smooth in structure, with minimal visible irregularities or distortions. The color gradient transitions from a yellowish core to a bluer, less intense outer region. This suggests some ongoing star formation within its outer disk. There is no clear evidence of a pronounced spiral arm structure or bar. Its overall appearance indicates that it is a quiescent galaxy, without significant major merger activity or tidal disturbances. The distribution of light is concentrated in the center with a gradual decline towards its periphery.
