The galaxy presents as a luminous, elongated structure. The central region exhibits a concentrated glow, appearing smooth and relatively featureless. The overall color profile indicates a higher concentration of older stellar populations. The galaxy displays an elliptical morphology, notably cigar-shaped with no readily apparent spiral arm structures. There appears to be little evidence of ongoing major merging events, although subtle asymmetries might suggest minor gravitational disturbances or tidal interactions. The overall appearance suggests a system with a moderate stellar mass and low star formation rate.
