The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth light distribution. The central region of the galaxy displays a higher concentration of luminosity, gradually decreasing towards the outer edges. The shape is elongated, closer to cigar shaped, indicating a non-spherical morphology. There is a subtle color gradient, with the central region appearing more yellow or golden. There is no strong evidence of significant spiral arm structure or ongoing major merger events. There is only mild evidence of minor disturbance, but overall the galaxy seems largely undisturbed. The light distribution is relatively uniform and lacks prominent features that would indicate active star formation regions. 
