This galaxy presents as a slightly inclined disk. The central bulge is bright and appears yellowish-orange in color, suggestive of an older stellar population. Moving outward from the bulge, the disk is less luminous and exhibits a bluer hue, potentially indicating ongoing star formation. The galaxy's overall shape is somewhere between round and elongated, possibly due to its inclination relative to our line of sight. There is no immediately obvious sign of strong tidal disturbances or major mergers. Some faint irregularities may be present in the outer disk, suggesting a possible minor interaction or internal activity. The galaxy does appear relatively smooth.
