The galaxy presents as a relatively smooth, elliptical morphology. It appears to be a fairly compact system, exhibiting a concentrated central bulge with a gradual decrease in luminosity towards the outer regions. The color profile suggests an older stellar population, with a yellowish hue dominating the central region, indicative of evolved stars. There is little evidence of distinct spiral arms or significant dust lanes, supporting the smooth morphology. Faint blue light in the outer edges may signify that there is some active star formation. It does not appear to be actively merging or undergoing major disturbances, although there are minor irregularities in the outskirts that could be indicative of interactions. The axial ratio suggests it is closer to being round than cigar-shaped. Overall, the galaxy appears to be a massive system with a relatively low star formation rate.
