The galaxy presents as a somewhat elliptical structure with a relatively smooth appearance overall, though some features are discernible. The central region exhibits a high degree of concentration, displaying a yellowish-orange hue, which may indicate an older stellar population. Moving outward from the core, there is a noticeable transition in color. Faint reddish patches are present on the lower half of the galaxy, these could indicate regions of on-going star formation activity or areas enriched with dust. Toward the upper portion of the galaxy, there appears to be a bluish tint, suggesting the presence of younger, hotter stars. The galaxy does not appear perfectly round, showing a slight elongation, and possibly some degree of tidal disturbance or interaction given the asymmetric distribution of star formation regions.
