The galaxy presents as a relatively smooth, elongated spheroid. The color is a yellowish-orange, suggesting an older stellar population and less ongoing star formation. There is no obvious spiral structure or distinct features, such as dust lanes or prominent star-forming regions. The galaxy appears to be mostly undisturbed, showing no strong signs of tidal interactions or recent mergers, although there is a slight elongation that could point to minor past interactions. The concentration of light is high towards the center, gradually decreasing outward, hinting at a higher density of stars in the galactic core.
