The galaxy presents as a relatively smooth, centrally concentrated object with a slightly elongated shape. It exhibits a central bulge that appears bright and yellowish, suggesting a population of older stars. Fainter, bluish light extends outwards from the bulge, potentially indicating regions of more recent star formation within the galactic disk. No obvious spiral arm structures are discernible. The overall structure suggests a relatively quiescent galaxy, possibly an elliptical or lenticular type, at a redshift of approximately 0.144.
