The galaxy presents as a relatively smooth and centrally concentrated object, with an overall elliptical morphology. The light distribution suggests a dominant spheroidal component, with a gradual decrease in intensity from the core outwards. There is little evidence of spiral arm structure. The galaxy's core appears to be more yellow-red in color, possibly indicating an older stellar population, surrounded by a bluer halo suggesting recent or ongoing star formation, albeit at a moderate level. There are no obvious signs of major mergers or significant tidal disturbances within the immediate vicinity of the galaxy. The ratio of the semi-major to semi-minor axes is approximately 0.8, suggesting a moderately elliptical shape. The overall color indices suggest that this galaxy is likely an intermediate type, between a pure elliptical and a pure spiral, with a mix of stellar populations and star-forming regions. The size indicates that the galaxy is a small to moderate size.
