The galaxy appears as a concentrated, luminous object with a generally smooth morphology. The core exhibits a bright, yellowish-white hue indicative of an older stellar population. The overall shape is predominantly round, with minimal apparent distortion. There is a suggestion of minor tidal interaction or disturbance, as evidenced by a faint, elongated structure extending outward from the main body on the left side. The main body exhibits a redder hue, possibly due to dust extinction or an older stellar population. There is no evidence of significant spiral arm structure or a prominent disk. The object appears to be a relatively massive system, likely with a quiescent star formation rate. Based on its morphology, the object is likely a relatively old, massive galaxy, probably on the red sequence.
