The galaxy presents a generally smooth morphology, with a centrally concentrated luminosity profile. The core exhibits a yellowish-white hue, potentially indicating an older stellar population. A faint, extended halo surrounds the central region, gradually fading into the background sky. The overall shape appears slightly elliptical, exhibiting an aspect ratio close to unity. There is a suggestion of very minor asymmetry in the outer halo, but no distinct features such as spiral arms, bars, or tidal tails are readily apparent. The galaxy's color suggests a moderately evolved system with a relatively low ongoing star formation rate. There is no evidence of significant dust extinction or recent merger activity based on the observed morphology.
