The galaxy presents as a relatively smooth, centrally concentrated object. It appears nearly circular in projection, exhibiting a high degree of central symmetry. There is a slight elongation, but the overall shape approximates a spheroid.

The color profile suggests the presence of a central, moderately bright bulge region, with a color index indicating a somewhat older stellar population and an active, but not overwhelmingly strong, star formation rate. No clear spiral arm structure is apparent. The galaxy shows no strong evidence of recent major merger activity, although there may be hints of minor tidal disturbances or interactions. The color gradient within the galaxy appears subtle, transitioning smoothly from the core to the outer regions.
