This galaxy appears to be an elliptical galaxy, exhibiting a generally smooth, featureless morphology. The light is concentrated towards the center, suggesting a dense galactic nucleus. The shape is somewhat elongated, but significantly departs from a spiral structure. There is a color gradient visible, transitioning from a yellow/orange hue in the center to slightly bluer tones in the outer regions. No obvious signs of spiral arms, dust lanes, or ongoing major mergers are apparent. The low level of visible blue light suggests that this galaxy has a relatively low star formation rate. Overall, this galaxy appears to be a relatively quiescent system with a dominant population of older stars. Some minor disturbances may be present in the galaxy, as it appears to not be perfectly smooth.