The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely elliptical, exhibiting a high degree of radial symmetry. The luminosity profile indicates a bright core, diminishing gradually towards the outer regions. The light distribution suggests a lack of significant spiral arm structures or prominent dust lanes. The galaxy exhibits a subtle color gradient, appearing yellower at the core and transitioning to a slightly bluer hue in the outskirts, indicative of differing stellar populations. There is no obvious evidence of ongoing major merging activity or significant tidal disturbances in the immediate vicinity of the galaxy. The overall appearance is consistent with an evolved galaxy, possibly a lenticular or elliptical type, with moderate star formation activity.
