The galaxy presents as a concentrated, luminous object with a generally smooth morphology. Its light is dominated by a yellow-orange hue centrally, suggestive of an older stellar population. There is a slight elongation, but generally it appears quite rounded. Faint, diffuse extensions are present, possibly indicating tidal interactions or a slight disturbance. The absence of well-defined spiral arms suggests a spheroidal or elliptical classification. Star formation appears minimal based on the color profile, pointing to a galaxy nearing the end of its star-forming activity.
