The galaxy presents an elongated, cigar-shaped morphology. Its light distribution appears relatively smooth, although there is a subtle color gradient evident. A bluer hue is observed in the outer regions, suggesting the presence of younger stellar populations and ongoing or recent star formation. The central region exhibits a more yellow-reddish color, indicative of an older stellar population. There is no clear evidence of spiral arm structure or significant dust lanes. The galaxy's smooth light profile is most likely an indication of its classification as an elliptical galaxy, but the color gradients show potential signs of star formation. There is a slight hint of interaction or minor disturbance within the galaxy.
