The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a centrally concentrated brightness profile. The core region is the most luminous, with the light gradually decreasing outwards. There appears to be minimal indication of distinct spiral arms or a prominent disk. The overall shape is generally round. The color profile appears somewhat uniform, exhibiting primarily warmer tones with a slight shift towards redder hues in the outer regions. There's no obvious evidence of ongoing major merging activity or significant tidal disturbances. The object appears to be an evolved system with a relatively low rate of star formation.
