The galaxy presents as an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. There is an apparent absence of spiral arms or prominent dust lanes. The galaxy’s color profile shows a yellowish-white hue in the central region, suggestive of an older stellar population. The outer regions gradually fade in intensity, with subtle hints of bluer tones, potentially indicating the presence of a younger, albeit limited, stellar population compared to the core. Based on visual inspection alone, there is no indication of tidal tails, strong distortions, or ongoing major merger events.
