The galaxy presents as a generally smooth, elliptical-like structure. It exhibits a noticeable elongation, appearing cigar-shaped rather than perfectly spherical. The color profile suggests a dominant population of older stars, evidenced by the reddish hue concentrated towards one end of the major axis. There is some indication of ongoing star formation, though subdued, as suggested by the subtle greenish-yellow tinge visible in the central region and extending along the primary axis. No distinct spiral arms or bar structures are discernible. There appears to be a minor asymmetry in the distribution of light intensity along the major axis, with one end possibly exhibiting a slightly higher concentration of luminous material. The overall morphology does not immediately suggest a major ongoing merger event, although subtle disturbances or tidal features cannot be entirely ruled out at this resolution. The galaxy has a generally quiescent star formation rate and is a fairly massive galaxy.