The galaxy appears as a somewhat rounded, luminous object. It exhibits a primarily smooth morphology with a concentrated central region. There is a suggestion of a slight elongation, though not dramatically cigar-shaped. The color profile indicates a redder hue with hints of green, suggesting a population of older stars and potentially the presence of dust obscuration. There is evidence of a possible interaction or merger event, as indicated by a subtle disturbance in its overall form. The overall light distribution suggests a substantial mass and potential for recent, but low levels of star formation activity.
