The galaxy presents a relatively smooth, elliptical morphology, with a dominant central bulge exhibiting a yellowish hue. This suggests an older stellar population residing within the bulge. The surrounding disk, while less prominent, shows hints of bluer, more actively star-forming regions, particularly on one side of the galaxy. A slight asymmetry is observed, with a possible tidal feature or minor disturbance manifesting as a faint extension, implying past or ongoing interactions. The round shape suggests we are viewing the galaxy close to face-on. Overall, the galaxy appears as a transition object with a bulge dominated by old stars.
