The galaxy appears as a moderately inclined, disk-shaped structure. The central region exhibits a concentrated luminosity, suggesting a prominent galactic bulge. The color distribution indicates a relatively red population, transitioning to slightly bluer hues towards the outer regions of the disk. The morphology leans towards a smooth appearance, though subtle features hint at the presence of a disk or spiral structure. The galaxy's overall shape is elongated, nearly cigar-shaped, indicating a significant inclination with respect to our line of sight. There is no obvious evidence of major mergers or strong tidal disturbances, though subtle irregularities might point to minor interactions. The galaxy shows a moderate level of star formation activity. 
