The galaxy presents as a somewhat elongated, though not perfectly elliptical, structure. Its major axis is estimated to be approximately 6 kpc. The galaxy's light appears to be concentrated towards the center, suggesting the presence of a bulge or core region. The color profile shows a tendency towards redder hues, particularly in the central regions, which could indicate a population of older stars and a lack of significant ongoing star formation, particularly when considered with the absolute magnitudes. There is a hint of bluer tones at the fringes of the object suggesting a star forming region. No strong spiral arm structures or dust lanes are immediately apparent. There appears to be no evidence of any major mergers or tidal disturbances affecting this object.
