The galaxy presents as a relatively smooth, elliptical structure, displaying a concentrated central bulge with a diffuse halo. The shape appears somewhat elongated, approaching a cigar-like form, though with softened edges. There is a subtle colour gradient observed across the galaxy, with the core exhibiting a slightly bluer hue, potentially indicating a region of younger stellar populations or ongoing star formation activity. However, the overall colour suggests an older stellar population is dominant. The absence of distinct spiral arms or significant dust lanes reinforces its classification as an elliptical galaxy, and there is no apparent major disturbance from mergers visible in the galaxy's morphology, though the possibility of minor interaction cannot be ruled out based on the image alone. The galaxy has a moderate estimated mass and a relatively low star formation rate. 
