The galaxy exhibits a generally elliptical morphology, presenting a disk-like structure with a noticeable bulge. The color profile of the galaxy is complex, with a bright, yellowish core surrounded by a greenish halo. This may indicate the presence of a stellar population gradient. The presence of green in the halo might suggest active star formation. There appears to be some disturbance in the structure, possibly indicating a tidal interaction or past merger. The bright central bulge is elongated along the major axis, which is indicative of the disk. There might be some disruption with a faint halo structure, suggesting a recent disturbance or interaction.
