The galaxy presents a relatively smooth and concentrated morphology. It exhibits a somewhat elliptical appearance, tending towards a rounded shape rather than a highly elongated or cigar-shaped form. Coloration appears complex, with a central region showing evidence of a yellower hue which could indicate an older stellar population. This is adjoined by a redder region that may be a zone of active star formation. The overall light distribution suggests a system dominated by a spheroidal component. The galaxy's apparent structure does not obviously present clear spiral arms or a well-defined disk. There are indications of a possible merger event in the form of tidal distortions, with at least two distinct clumps of light present. This could mean that the galaxy is in the process of merging with another object.
