The galaxy presents as a moderately luminous, elongated structure. It exhibits a generally smooth morphology, with a lack of defined spiral arms or distinct features. The color profile suggests a mixture of stellar populations. A central region of the galaxy displays a yellowish hue, possibly indicative of older, cooler stars or dust concentration. This core gradually transitions to a greenish-blue tint in the outer regions, which may be indicative of some star formation, although the extent of star formation appears to be modest. Overall, the galaxy's structure appears relatively undisturbed, showing no signs of ongoing major mergers or significant tidal interactions. The general shape suggests a likely elliptical or lenticular classification.