The galaxy presents as a single, relatively smooth, and concentrated light source. The morphology appears largely spheroidal, exhibiting a distinct central bulge with a yellowish hue, suggestive of an older stellar population. There is minimal evidence of spiral arm structure or significant dust lanes. The overall color profile leans towards the redder end of the spectrum, potentially indicating lower levels of ongoing star formation. There is a slight elongation, but for the most part it can be described as round to in-between. No obvious signs of recent merger activity or tidal disturbances are visible.
