The galaxy presents as an elliptical morphology, appearing relatively smooth and featureless. The central region exhibits a higher surface brightness, gradually fading towards the outer edges of the galaxy. The shape appears elongated, with the major axis significantly longer than the minor axis, resulting in a cigar-like appearance. There is a suggestion of slight disturbance in the galactic structure, potentially indicating a minor interaction or past merger event, but the overall structure remains largely undisturbed. There is faint color variation across the galaxy, with the central regions exhibiting a slightly bluer hue compared to the redder outer regions. Star formation appears suppressed, leading to a dominant population of older stars. The galaxy is likely a relatively low-mass system.