The galaxy appears as a centrally concentrated object with a relatively smooth morphology. There is evidence of a weak disk structure, though this is not a dominant feature. Its roundness suggests it is not highly inclined with respect to our line of sight. There is some indication of minor disturbances in its morphology; potentially tidal tails, but it could be a minor merger event. The galaxy exhibits a color gradient from the center to the outer regions. The central region shows yellow and green color, shifting to redder hues in the outer portions of the galaxy. This may be related to the age or metallicity of the stellar populations in these regions.