The galaxy presents as a concentrated, somewhat symmetrical object, exhibiting a central bulge of moderate luminosity. There is evidence of a flattened disk component, but it is not sharply defined and possesses a relatively smooth texture. The color profile suggests a population of older stars, with a reddish-yellow hue dominating the central regions. No distinct spiral arms are visible. There are some indications of possible minor tidal disturbances or interactions with other bodies, but this is uncertain.
