This galaxy presents as a disk galaxy, likely observed at a high inclination angle, near edge-on. The central bulge appears bright and prominent, exhibiting a somewhat spheroidal shape. The disk component is visible as a flattened structure extending outwards from the bulge. There's evidence of possible dust lanes within the disk, although their structure is somewhat obscured by the inclination angle and image quality. The color profile shows a trend towards bluer hues in the outer regions of the disk, possibly indicating active star formation in these areas, while the central bulge exhibits redder tones, characteristic of an older stellar population. There may be some disturbances in the overall structure, possibly indicating minor tidal interactions. The object is relatively isolated within its field, showing no signs of a major merger.