The galaxy presents as a moderately luminous system, exhibiting a pronounced central bulge that graduates smoothly outwards. The overall shape is elliptical, appearing somewhat elongated along a single axis, trending towards a cigar-like form. There is a subtle color gradient, with the core appearing more yellow-white, suggestive of an older stellar population. A faint disk-like structure can be inferred, but no distinct spiral arms or prominent star-forming regions are visible within the galaxy's morphology. There appears to be no major ongoing merger activity or significant tidal disturbances affecting the galaxy's structure, though a minor irregularity on one side cannot be ruled out.
