The galaxy presents as a moderately luminous, elliptical galaxy with a relatively smooth morphology. It exhibits a yellowish-orange hue, suggesting an older stellar population with reduced active star formation. The galaxy is characterized by a concentrated central bulge, which gradually diffuses outward into an extended halo. A slight elongation is visible along its primary axis, deviating subtly from a perfectly circular shape. Some faint, irregular features or tidal streams may be present, hinting at possible past interactions or mergers. Overall, the galaxy appears to be relatively isolated with no prominent signs of ongoing major merging activity, though minor disturbances cannot be ruled out. Its size indicates it is a relatively massive system.
