The galaxy presents as an edge-on spiral, characterized by a flattened disk structure. A distinct central bulge is visible, exhibiting a smooth, concentrated distribution of light, with an apparent spheroidal shape. The bulge appears to be a significant contributor to the overall luminosity of the galaxy. The disk component is relatively thin, with a subtle gradient in surface brightness extending outward from the bulge. There is no obvious spiral structure. No signs of ongoing merger activity or significant tidal disturbances are evident in the immediate vicinity of the galaxy. The galaxy's color is redshifted, indicating a population of older stars with a low rate of star formation.
