The galaxy presents as a roughly elliptical, moderately concentrated light source with an apparent axis ratio close to unity, suggesting it is nearly face-on. The color profile exhibits a yellowish-white core that transitions to a reddish outer region. There are no readily discernible spiral arms or prominent dust lanes. The overall morphology suggests a relatively smooth distribution of stellar populations. The galaxy appears relatively isolated, showing no signs of ongoing major merger activity or significant tidal distortions, although a slight asymmetry cannot be ruled out. Given the apparent color and smooth morphology, it is likely an early-type galaxy, possibly an elliptical or lenticular galaxy, with moderate stellar mass and star formation activity.
