The galaxy presents as a relatively smooth, elliptical structure, with a high degree of central concentration. The core region exhibits a yellowish hue, possibly indicating an older stellar population. Moving outwards from the center, the galaxy's color shifts to a slightly bluer tint. This may suggest a presence of younger, bluer stars in the outer regions, or perhaps regions of more active star formation.

The galaxy's overall shape is elongated, appearing cigar-shaped. There is no evidence of strong tidal disturbances or major mergers in its immediate vicinity, however there is very slight disturbance observed that could possibly be due to a minor merger event in the past. There appears to be a faint extended halo around the galaxy, though the signal is weak.
