The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology. The light profile appears to diminish gradually from a bright core region. There is a slight elongation visible in the structure, deviating from a perfectly circular shape, though it's not highly pronounced.

In terms of color distribution, the central region is distinctly bluer compared to the outer regions which appear slightly redder. This could indicate a difference in stellar populations, with younger, hotter stars dominating the core, and older, cooler stars residing in the outskirts. No obvious spiral arm structures or prominent dust lanes are observed. There is no indication of any major merger events.
