This galaxy presents as a somewhat elongated, lenticular or early spiral type system. The central bulge exhibits a concentrated, yellowish-white luminosity, suggesting a population of older stars. Fainter, blue tinged spiral arms appear tightly wound around the central bulge, indicating on-going, but perhaps subdued star formation. The disk component shows evidence of dust lanes or obscured regions, particularly along the edges. Overall, the galaxy exhibits a relatively smooth, consolidated structure, with minimal signs of significant tidal disturbances or ongoing major mergers. It seems to be an intermediate mass galaxy with a moderate star formation rate. The galaxy's morphology leans towards a transitional stage between elliptical and spiral galaxies. There is no definite nucleus. 
