The galaxy presents as a relatively smooth, elliptical morphology. The color profile suggests a dominant population of older stars, exhibiting a yellowish-red hue in the central regions. A slight blue tinge towards the outer edges may indicate pockets of younger, hotter stars, but overall star formation appears to be suppressed. The galaxy exhibits minimal signs of spiral arm structure or prominent dust lanes, with no signs of merging or tidal disruption. It has a slightly elongated shape and a relatively high central surface brightness.
