The galaxy presents as a relatively smooth object, with a central, bright bulge region that dominates the overall luminosity. Faint, diffuse features are visible, suggesting a possible disk component, though it lacks defined spiral arm structures. The shape appears generally elliptical to moderately rounded. There might be subtle signs of a minor disturbance or interaction, based on irregularities in the outer regions. The color profile suggests a mix of stellar populations, with the central bulge exhibiting a more yellow hue, potentially indicating an older stellar population, while the disk component shows bluer regions suggestive of ongoing or recent star formation. Overall, the galaxy appears to be a mid-mass system, showing characteristics transitioning between elliptical and spiral types.
