The galaxy presents as a relatively smooth, somewhat rounded object. It appears to have a concentrated central bulge that appears yellow/orange in color, suggesting an older stellar population. There is a slight flattening observed, but there are no distinct spiral arms or significant disk structures discernible in this image. The galaxy exhibits a relatively high degree of central concentration with a smooth appearance, implying a possible early-type, elliptical classification or potentially a late-stage spiral galaxy with a dominant bulge. There are no apparent signs of recent or ongoing major mergers, tidal disturbances or active star formation regions visually detected within the galaxy.