The galaxy appears to be a relatively smooth, early-type system, potentially an elliptical galaxy. The light profile shows a centrally concentrated bulge with a diffuse halo extending outwards. There's little evidence of distinct spiral arms or significant dust lanes. The core exhibits a yellowish hue, indicative of an older stellar population. The outer regions appear slightly bluer, suggesting some ongoing, albeit low, star formation. The galaxy's overall shape is elongated, but not extremely so, appearing as an intermediate elliptical form. There is no apparent evidence of a major merger or significant tidal disturbance, although subtle irregularities in the outer halo cannot be ruled out without further investigation.
