The galaxy presents an overall elliptical morphology, appearing relatively compact with a noticeable tidal tail extending from its lower region. The central region exhibits a bright, concentrated core, possibly indicative of an active galactic nucleus or a dense stellar population. Surrounding this core is a less defined, diffuse halo of bluish light, suggesting the presence of younger, hotter stars or active star formation. The tidal tail displays a reddish-orange hue, implying an older stellar population or dust obscuration along its extent. There are some suggestions of potential interaction or disturbance in the galaxy's structure beyond the tidal tail; however, the image resolution limits the certainty of this assessment. Further spectroscopic analysis would be required to determine the composition and dynamics of this galaxy.
