The galaxy presents as a centrally concentrated object with a generally smooth morphology. It exhibits a slightly elongated profile. The central region displays a bright, diffuse glow, which fades toward the outer edges. There appears to be evidence of a possible ongoing or recent merger event, characterized by a disturbed structure and diffuse distribution of the galaxy. The lack of significant dust lanes or prominent spiral arm structures is notable, suggesting the galaxy is relatively evolved. The light profile and color indices suggest a redder color, likely indicative of an older stellar population and suppressed star formation activity.
