The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge region, surrounded by a more diffuse halo. The color profile suggests a dominant population of older stars, with a relatively low rate of current star formation.  There's potential evidence of minor tidal disturbances, potentially indicating past or ongoing interactions with smaller companion galaxies or gravitational interactions, though the overall structure does not suggest an ongoing major merger. The galaxy shows a intermediate degree of roundness.
