The galaxy presents as a somewhat elliptical, lenticular morphology. The central bulge region exhibits a bright, concentrated luminosity, appearing yellow-white. The surrounding disk is less defined, with a fainter, bluish-white hue, potentially indicating regions of younger stellar populations and ongoing star formation. There is a noticeable lack of spiral arm structures and no obvious signs of a bar. The overall appearance suggests a relatively smooth structure with no strong evidence of recent or ongoing major mergers or significant tidal disturbances. The galaxy appears primarily smooth and moderately concentrated.
