This galaxy presents as a relatively smooth, centrally concentrated object with a generally round morphology. There is no obvious spiral structure or bar visible in this image. The color gradient suggests a slightly yellower core, possibly indicative of an older stellar population concentrated towards the center. Fainter, bluer emission is observed in the outer regions of the galaxy, suggestive of recent or ongoing star formation. There appears to be no significant tidal disturbance or evidence of a major merger event in its recent history.
