The galaxy presents an elongated, cigar-shaped morphology. Its light profile appears relatively smooth and centrally concentrated, with a gradual decrease in intensity towards the outer edges. The central region exhibits a yellowish-orange hue, suggestive of an older stellar population. Fainter blue regions are present closer to the periphery which may indicate some recent star formation. There is no obvious spiral arm structure or prominent dust lanes. The galaxy appears isolated, showing no immediate signs of tidal distortion or interaction with other galaxies.
