The galaxy presents an overall smooth morphology, suggestive of an elliptical or lenticular classification. The central region exhibits a bright, concentrated core, surrounded by a more diffuse halo. The galaxy's shape appears to be generally elliptical. There's a slight elongation, possibly leaning towards a cigar shape. A noticeable color gradient is apparent, with the core exhibiting a bluer hue which may indicate a population of younger stars. Moving outwards from the core, the color shifts towards redder tones, possibly indicating older stellar populations. There is a notable feature that suggests a possible interaction or merger event. A portion of the galaxy appears heavily disturbed, and elongated with a strong color gradient. This may be tidal debris, which could explain the smooth morphology mixed with disturbed morphology.
