The galaxy presents a somewhat elongated, cigar-shaped morphology. It appears largely smooth in texture with a bright central bulge that gradually fades towards its outer edges. The color distribution suggests an aging stellar population, with a bluer hue concentrated in the central region and a shift toward redder tones in the outer regions. There is no indication of a distinct spiral arm structure or significant dust lanes. Overall, the galaxy exhibits characteristics consistent with an elliptical or lenticular galaxy, with a moderate amount of on-going or recent star formation primarily located within the nucleus. There is some sign of possible minor disturbance, but it is unlikely to be undergoing a major merger or tidal interaction.
