The galaxy presents a predominantly smooth morphology, indicating an elliptical or lenticular classification. The light profile appears concentrated towards the center, suggesting a spheroidal structure with an aging stellar population. The color gradient transitions from a yellowish-orange hue at the core to a slightly bluer tint in the outer regions, possibly indicating ongoing, albeit diminished, star formation activity in its outskirts. While it mainly appears undisturbed, a minor asymmetry in its shape might indicate past or ongoing interactions with another celestial object. Its elongation suggests a possible cigar shape. No prominent spiral arms or distinct features such as dust lanes are observed.
