The galaxy presents as a moderately bright, elongated structure with a discernible bulge. The light distribution appears relatively smooth, suggesting a lack of prominent spiral arms or significant dust lanes. The central region exhibits a yellowish hue, potentially indicating an older stellar population. The outer regions transition to a bluer color, perhaps signifying more recent star formation activity. There is a suggestion of a faint disk component, but the overall morphology is dominated by a spheroidal shape. The galaxy's shape appears close to being cigar-shaped rather than close to round. No obvious signs of a major ongoing merger or significant tidal disturbance are visible.
