The galaxy appears to be elliptical in morphology, exhibiting a generally smooth light distribution. The central region is noticeably brighter and more concentrated than the outer regions, indicating a possible central bulge. There is a slight elongation to the shape, with the galaxy appearing to be more "in-between" shaped rather than perfectly round, with a somewhat irregular morphology. The color gradient suggests an older stellar population with a reddish hue in the central region, transitioning to a slightly bluer color in the outer regions. There is no obvious presence of spiral arms or significant dust lanes. There are no signs of any major disturbances or merging events; however, there is a slight irregularity which may suggest minor disturbance or interaction. Overall, this galaxy appears to be a moderately massive elliptical galaxy with a moderate amount of star formation occurring within its boundaries.