This galaxy presents as a relatively smooth, elliptical morphology. There is a notable lack of distinct spiral arms or bar-like structures, which suggests a more spheroidal stellar distribution. The galaxy exhibits a concentrated central bulge that dominates its overall luminosity. The color gradient appears to shift from a more yellowish core to slightly redder outer regions, potentially indicating an older stellar population in the central region. The galaxy's shape is elongated, appearing cigar-shaped rather than perfectly circular. There is no strong evidence of ongoing major mergers or significant tidal disturbances, although minor asymmetry cannot be ruled out based on this image alone. Star formation appears suppressed overall.
