The galaxy presents as a moderately luminous object with a generally smooth morphology. Its light is dominated by a central, concentrated bulge exhibiting a yellowish hue. The surrounding regions display a fainter, more diffuse emission with hints of bluer color. There is little evidence of distinct spiral arms or significant dust lanes, suggesting a relatively evolved stellar population and a limited amount of on-going star formation. The galaxy exhibits a somewhat rounded appearance, with a slight ellipticity. No major signs of mergers or tidal disturbances are visible within the limits of the data. The overall impression is of a galaxy transitioning towards a later-type classification.
