The galaxy presents as a lenticular or early spiral type, exhibiting a generally smooth, elliptical morphology. It appears elongated, with an axial ratio indicating a significant degree of flattening. Some asymmetry is visible, suggesting possible tidal interactions or minor disturbances. The galaxy's light profile is centrally concentrated, typical of galaxies with a prominent bulge component. There is a subtle color gradient, with the central regions appearing slightly redder than the outer disk. The galaxy seems relatively isolated, showing no strong evidence of ongoing major mergers or interactions, however there may be signs of minor disturbance. There is no clear disk structure, but an absence of defined spiral arms suggests the galaxy is relatively quiescent in terms of recent star formation.
