The galaxy presents a somewhat smooth, elliptical morphology. Its overall shape is slightly elongated, appearing more "in-between" rather than perfectly round or cigar-shaped. There are some faint features that indicate a possible disk component, but they are not very prominent. The color profile suggests a mix of stellar populations; a dominant central bulge with older, redder stars surrounded by a disk with some bluer, younger stars. There may be some evidence of minor disturbance or interaction, suggesting potential recent merger activity or tidal interactions with neighboring galaxies, but it is not a strong merger. Star formation rate is low, with a considerable specific star formation rate. Overall, it's likely a massive galaxy undergoing a transition phase.
