The galaxy presents a generally elliptical morphology, appearing elongated or cigar-shaped. It exhibits a bright central bulge that appears smooth in texture, gradually fading into a less defined disk component. There may be subtle signs of tidal disturbances or minor asymmetries in the outer regions of the galaxy, possibly indicating past or ongoing interactions with other galaxies. The color profile suggests a diverse stellar population, with the central bulge appearing relatively redder, possibly indicating older stars, and the outer regions showing bluer hues, suggesting the presence of younger stars and active star formation. There is a relatively small amount of dust obscuration visible in the galaxy.
