This galaxy exhibits a generally elliptical morphology with a relatively smooth appearance, suggesting it is likely an early-type galaxy. There is a notable concentration of light towards the galactic center, indicating a dense core. The light distribution appears mostly uniform across the galaxy's extent, with a subtle decrease in brightness towards the edges. The galaxy's color profile suggests a mix of stellar populations, with perhaps a slightly redder hue in the central regions compared to the outer regions. This could indicate a higher concentration of older stars and a relatively low rate of ongoing star formation within the galaxy, although some blue regions would suggest recent star formation. There are no obvious spiral arm structures or significant dust lanes visible, further reinforcing the smooth, elliptical classification. Finally, there are no nearby companions to suggest that this galaxy is currently undergoing a major merger.
