The galaxy presents a generally elliptical morphology, appearing flattened along its minor axis. The light distribution suggests a centrally concentrated spheroid. The color gradient transitions from a yellowish-white core to a fainter, bluer outer region. Although difficult to discern, there may be subtle hints of spiral structure in the outer disk, but is still not very structured. The central bulge region appears more uniform and lacks noticeable dust lanes or distinct star-forming regions. The outskirts of the galaxy fade gradually into the background, indicating a relatively smooth density profile. There appears to be some disturbance to the light around the galaxy. The galaxy appears relatively isolated, lacking close companions or signs of ongoing major mergers.