The galaxy presents a largely smooth morphology, appearing elliptical in shape, with an approximate apparent axial ratio of 2:3. Its color profile suggests a relatively evolved stellar population, exhibiting a yellowish hue, consistent with a dominance of older, less massive stars. There are no strong indications of distinct spiral arms or significant dust lanes. The galaxy’s light distribution is concentrated towards the center, with a gradual decrease in intensity towards the outer regions. There is little evidence of ongoing major star formation; any star formation activity is likely subdued. There are no distinct tidal features or nearby companion galaxies visibly interacting, which supports the likelihood of a dynamically relaxed state. There is a slight, but not distinct, blue shift at its edges, indicating the presence of potential new, yet small, star formation.
