The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears to be largely spheroidal, with a high degree of roundness. There is a lack of prominent spiral arms or bar structures, suggesting a classification towards the elliptical end of the Hubble sequence, or potentially a lenticular galaxy viewed face-on. The light distribution is fairly uniform, with a gentle gradient from the center outwards.

There are no obvious signs of a recent major merger event, although minor disturbances or tidal features cannot be ruled out at this resolution. The color profile indicates a bias toward older stellar populations, as evidenced by the redder hues in some regions, but there is also evidence of some star formation, as indicated by the somewhat bluer color, particularly in the central region. The galaxy's overall luminosity appears moderate.
