The galaxy presents as a somewhat smooth, disk-like structure with an intermediate ellipticity. The central bulge exhibits a yellowish hue, suggesting an older stellar population, while the outer disk appears bluer, potentially indicating more recent star formation. There is evidence of some distortion or minor disturbances in the disk, possibly related to interactions or internal dynamics. The overall shape is neither perfectly round nor elongated into a cigar shape, appearing somewhere in between. No signs of major merger events are immediately apparent, but signs of possible disturbances indicate some sort of activity.