The galaxy presents as an elongated, cigar-shaped structure. The central region exhibits a concentrated luminosity with a yellowish-white hue, suggesting a population of older stars. Progressing outward from the core, a diffuse bluish halo is observed, possibly indicative of a younger stellar population or ongoing star formation. The smooth texture and lack of distinct spiral arms suggest a classification towards the elliptical or lenticular end of the Hubble sequence. There is a subtle hint of asymmetry or a minor perturbation in the galaxy's structure, although no obvious signs of a major merger are apparent. The absence of prominent dust lanes further supports the possibility of it being a relatively quiescent galaxy.
