The galaxy presents a generally smooth and rounded morphology. There appears to be no distinct disk structure or spiral arms visible in this image, nor does there appear to be any bar. The color distribution is suggestive of an older stellar population, with a concentration of yellowish-orange light in the central region. The overall luminosity profile suggests a centrally concentrated object, potentially an elliptical galaxy. There are no strong indications of ongoing major merger activity or significant tidal disturbances. Faint, diffuse emission may be present in the outer regions, but it lacks clear structure. The absence of strong blue colors indicates a relatively low rate of star formation.
