The galaxy presents as a generally smooth structure, with a concentrated central bulge.  The overall shape is somewhat elliptical, trending towards "in between" round and cigar shaped. There is little evidence of spiral arm structures or significant dust lanes within the disk or around the bulge.  The color appears relatively uniform, with a slightly yellower hue in the central region, suggesting an older stellar population concentrated in the bulge. No major merging or tidal disturbance is clearly visible, though there may be a faint indication of a minor disturbance or interaction based on a slight asymmetry in the outer regions.  The object appears to be relatively quiescent based on these morphological characteristics.
