The galaxy presents a primarily smooth, elliptical morphology. It appears to be moderately rounded, exhibiting a diffuse, centrally concentrated luminosity profile. There is evidence of a possible minor interaction or disturbance in the form of a small luminous patch located off-center. The galaxy exhibits colors indicating moderate star formation activity. Specifically, bluer regions are visible in the central area, suggesting the presence of younger, hotter stars, while the more extended features show redder hues, potentially indicative of an older stellar population. There may be indications of a merging event or some other disruption given the observed features. Overall, this appears to be a galaxy with an intermediate mass and moderate levels of star formation.
