The galaxy presents as an elliptical morphology, exhibiting a smooth light distribution without any prominent spiral arms or bar structure. The central bulge region appears to be a concentrated source of light with a yellowish hue, possibly indicative of an older stellar population. The outer regions of the galaxy fade gradually into the background, showing a diffuse halo. There is a slight asymmetry to the galaxy's overall shape; with a slight distortion towards the lower left. The color gradients suggest a radial change in stellar populations, moving from older populations in the centre, to areas with sparse pockets of younger stars in the outskirt regions. There is no indication of significant ongoing star formation within the galaxy. Based on the light distribution, this appears to be a relatively quiescent galaxy, with no signs of major disturbances or interactions with other galaxies.
