The galaxy appears as an elliptical-like structure, exhibiting a relatively smooth, featureless morphology. Its shape is elongated, resembling a cigar, although it is not extremely so. The light distribution is concentrated toward the center, indicating a prominent galactic bulge. A subtle color gradient can be observed, with a bluish hue toward one end, potentially suggesting regions of active star formation. Redder regions at the opposite end may indicate an older stellar population or dust obscuration. There is a slight asymmetry in the outer regions, hinting at a possible minor interaction or tidal disturbance, although no clear merging features are visible. The galaxy exhibits a moderate level of star formation activity, and has an approximate size of 4.4 kpc. The estimated mass indicates that this galaxy is of significant size.
