The galaxy presents as an elongated, cigar-shaped structure. Its central region exhibits a concentrated, bright luminosity, with a yellowish-white hue, suggesting an older stellar population. The light gradually fades towards the edges, and the overall color shifts to a slightly redder tone, possibly indicating the presence of dust lanes or a population of cooler stars in the outer regions. There is no strong evidence of distinct spiral arms, indicating that the galaxy is likely an elliptical or lenticular type. No significant tidal distortions or interactions with other galaxies are visible in its immediate vicinity, suggesting it may be relatively isolated, and that no major merging has occurred recently.
