The observed galaxy presents as a relatively smooth, centrally concentrated object. Its overall color profile leans towards the blue end of the spectrum. The morphology appears largely elliptical, exhibiting a generally rounded shape. There is a slight asymmetry detectable in the outer regions. No distinct spiral arms or bar structures are clearly visible. There is weak evidence of a subtle disturbance in the overall structure of the galaxy; some regions exhibit a slight blurring or irregularity. The central bulge appears prominent and luminous, with a gradual decline in brightness toward the outer edges. Overall, the galaxy does not seem to be undergoing any major merging activity.
