The galaxy presents as a relatively smooth, elliptical structure. Its morphology is somewhat elongated, appearing cigar-shaped rather than perfectly round. The central region exhibits a strong concentration of light, suggesting a prominent galactic bulge. Moving outward from the core, the light intensity gradually decreases.  The overall color appears yellowish, indicating a population of older stars and a low rate of ongoing star formation.  There is little evidence of spiral arms or significant dust lanes.  No major merging activity or significant tidal disturbances are apparent in the surrounding regions of the galaxy.
