The galaxy presents an elliptical morphology, appearing as a smooth, centrally concentrated luminosity profile. It exhibits a relatively symmetrical shape, tending towards being cigar-shaped in appearance. The light distribution suggests a well-mixed stellar population with a dominant older population, consistent with low star formation activity. The overall color is relatively red, indicative of older stellar populations and potentially higher dust content. There is no evidence of distinct spiral arms or a well-defined disk. No major merger events or significant tidal disturbances are apparent, though subtle irregularities at the periphery cannot be entirely ruled out at this resolution.
